Constellation Scorpius (Scorpion)

Properties

Despite an area of 497 square degrees, Scorpius is a large, bright and impressive constellation and is one of the most beautiful in the sky. It is partially located in the band of the Milky Way, near its center, west of Sagittarius. The outlines of this constellation are very reminiscent of the shape of this animal: the threateningly outstretched claws lie in the constellation Libra; the striking star formation around Antares, the heart of the scorpion, represents the breastplate; even the tail with the poison sting, raised to attack, is indicated by a star bow. The center of the constellation culminates around midnight on June 3rd. ^{[9, 15]}

Stars with Proper Names:

α Sco: Antares, Cor Scorpii, Kalb Al Akrab, Vespertilio
β¹ Sco: Graffias, Grafias, Grassias, Acrab, Akrab, Elacrab
δ Sco: Dschubba, Iclarkrau
θ Sco: Sargas
λ Sco: Shaula
ν Sco: Jabbah
σ Sco: Alniyat, Al Niyat
υ Sco: Lesath, Lesuth

Data for constellation Scorpius ^[150]
IAU Name	Scorpius
IAU Genitive	Scorpii
IAU Abbr.	Sco
English Name	Scorpion
Season (47° N)	April … August
Right Ascension	15^h 47^m 15^s … 17^h 59^m 14^s
Declination	-45° 46' 01" … -08° 17' 45"
Area	497 deg²
Neighbours (N↻)	Oph, Lib, Lup, Nor, Ara, CrA, Sgr

Deep-Sky Object Descriptions

IC 4605

Messier 4

Butterfly Cluster
Messier 6

Cat's Paw Nebula
NGC 6334

NGC 6444

NGC 6453

Sh 2-9

Mythology and History

According to rock carvings in the Caucasus region, the constellation of Scorpio was already in the 3rd millennium BC. Known, but the scorpion also appears in the Orion legend:

Orion was a mighty hunter who knew how to captivate even goddesses in love because of his beautiful figure. Jealousy and resentment were the result, which finally cost the Orion his life. In another version of death, the scorpion plays a role. Gäa, the earth goddess sent Orion a poisonous scorpion because he bragged that there was no animal he could not kill. Orion is said to have died of a scorpion sting, or the Sagittarius came to him just in time Help? As a punishment, the scorpion was moved to a place in the sky that is almost exactly opposite the Orion, so that Orion rises when the scorpion goes down. ^[20]

The ancient Greeks counted the area, where today the constellation Libra is located, still to Scorpius and saw here the claws of the scorpion. This is the origin of the Arabic names of the stars. During Julius Caesar's lifetime, the Romans separated into this area and formed the independent constellation and zodiac sign Libra.

Indians from central Brazil see the Scorpion as a carrying net for children. Indians from the Rio Negro river basin in northern Brazil see the scorpion as a big snake with a wide open mouth and a twisted body. The bright Antares is the snake's prey to be strangled down. At the end of the tail lies the egg of the snake. ^[20] The Indians of the North American tribe of the Navajo interpreted the four stars, which form the stache of the scorpion, as the footprint of a running hare. The first appearance of this constellation at dawn heralded the approach of spring. ^{[61, 107]}

Catalogs

Yale Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991) ^[154]
HR	B	F	DM	HD	SAO	FK5	IR	M*	ADS	VarID	RA	Dec	vMag	spType	dMag	Sep ["]	Remarks
HR 5885		1	CD-2511131	141637	183854						15 50 58.7	-25 45 05	4.64	B3V			G:Sco OB2 assoc.; probable member of Sco-Cen cluster; upper Sco region; embedded in reflection nebulosity; member of,G:Pleiades group.,RV:Rapidly rotating star which might become Be star.
HR 5904		2	CD-2412352	142114	183896				9823		15 53 36.7	-25 19 38	4.59	B2.5Vn	2.5	2.3	D:CPM. Combined mag., color.,G:Sco OB2; Sco-Cen assoc.; probable member of Sco-Cen cluster; upper Sco region; embedded in reflection nebulosity.,RV:Rapidly rotating star which may become Be star.
HR 5906			CD-2412354	142165	183900			D			15 53 53.8	-24 31 59	5.39	B6IVn			D:Suspected occultation double.,G:Sco OB2; Sco-Cen assoc.; doubtful member of the Sco-Cen cluster; upper Sco region.
HR 5907			CD-2312569	142184	183901					7314	15 53 55.8	-23 58 41	5.42	B2.5Vne			G:Sco-Cen assoc.; doubtful member of the Sco-Cen cluster; upper Sco region.,VAR:Amp. 0.03V on time scale 2 hrs. suspected.
HR 5910			CD-2611096	142250	183907						15 54 30.0	-27 20 19	6.14	B6Vp			G:Sco OB2.,RV:Determinations of vsini range from 29 to 196k/s.
HR 5912		3	CD-2412365	142301	183914					V927 Sco	15 54 39.5	-25 14 37	5.87	B8IIIp			G:Sco OB2.,S:Helium-weak star.,VAR:1.45937d. Magnetic field variable 1.45955d (Landstreet et al. 1979, MNRAS, 188, 609).
HR 5917		4	CD-2511190	142445	183931						15 55 30.1	-26 15 57	5.62	A3V
HR 5928	ρ	5	CD-2811714	142669	183957	3258			9846		15 56 53.1	-29 12 51	3.88	B2IV-V	8.8	38.3	G:Sco OB2; Sco-Cen cluster; upper Sco region; member of Pleiades group.
HR 5934			BD-20 4364	142883	183972					7359	15 57 40.4	-20 58 59	5.85	B3V			G:Sco OB2; upper Sco complex.,SB:Large amp. Secondary much fainter.,VAR:Beta C?, 5.84 - 5.87V, 0.2872d.
HR 5942			CD-2412427	142990	183982					V913 Sco	15 58 34.8	-24 49 53	5.43	B5IV v			G:Sco OB2; Sco-Cen cluster; upper Sco region.,RV:vsini 200k/s.,S:He strong?,VAR:Small amp. in y. 0.492d or 0.976d. Also spectrum var.
HR 5944	π	6	CD-2511228	143018	183987	592			9862	7371	15 58 51.1	-26 06 51	2.89	B1V+B2V	1.2	0.0	C:Color excess E(B-V) = +0.08.,D:Primary is SB, 3.4, 6.4v sep. 0.0003"; third component, ADS 9862B, 12.2v at 50". vsini both A and B =<100k/s.,D:Component B, F4V, optical.,G:Sco OB2; Sco-Cen cluster; in HII region; upper Sco region; member of Pleiades group; in reflection nebula; member assoc.,G:Sco R1 at 145 pc.,SB:ADS 9862A, B1V, B2V, 1.5701d, K 131k/s, V0 -4k/s, msin3i 3.46, asini 2.83. Equal components.
HR 5953	δ	7	BD-22 4068	143275	184014	594	I	S			16 00 20.0	-22 37 18	2.32	B0.3IV	0.2	0.2	C:Color excess E(B-V) = +0.16. Conspicuous infrared deficiency.,D:Possible quadruple system: SB 3.0, 5.0v, sep. 0.00001", 3.3v at 0.1", and 4.9v at 0.186".,G:Sco OB2; Sco-Cen cluster; upper Sco region; HII region.,N:Dschubba; Iclarkrau.,R:Diam. = 0.00045 - 0.00046".,SB:Primary SB about 20d. Another companion 4.9v at 0.181", discovered by occultation and speckle interferometry, has,SB:longer period. Resolved by speckle observations 1986.45, sep. 0.17".
HR 5965			CD-2811817	143619	184049				9896		16 02 39.4	-29 08 09	6.03	K3III	6.8	11.0
HR 5969			CD-2511295	143787	184068		I				16 03 20.6	-25 51 55	5.00	K5III			G:Probable Hyades group.,R:Occultation diameter measure indicates point source.
HR 5973			CD-2412499	143900	184075		I				16 03 54.7	-24 43 35	6.21	K0
HR 5977	ξ		BD-10 4237	144069	159665				9909 B		16 04 22.1	-11 22 23	5.07 H	F5IV	0.2	1.2	D:Binary with HR 5978, q.v.,DYN:0.038".
HR 5978	ξ		BD-10 4237	144070	159665				9909 A		16 04 22.1	-11 22 23	4.77 H	F5IV	0.2	1.2	D:Quintuple system ADS 9909A-C is CPM with ADS 9910, 7.4 G8V, 8.1K0V sep. 11" at 281" from ADS 9909A. ADS 9909AB 4.9 F5IV,,D:4.9 F5IV, 45.69y, a = 0.720". Combined mag. 4.16V, combined colors. ADS 9909C, 7.30V, +0.75(B-V), dG7 at 7", physical.,DYN:0.038".,N:Has been called Grafias, a name more commonly applied to HR 5984.,SB:ADS 9909A, 44.70 yrs. K 3.7k/s, V0 -29.4k/s, asini 549. Period from visual double orbit.
HR 5984	β¹	8	BD-19 4307	144217	159682	597	I		9913 A	7424	16 05 26.2	-19 48 20	2.62	B1V	1.3	0.0	D:CPM with HR 5985 = ADS 9913C, at 14" and with B, 5.9v at 0.5", possibly SB. Lunar occultations and speckle,D:interferometry indicate companions 4.2v at 0.001" from A and 7.6v at 0.129" from C. Occultations by Jupiter and Io in,D:1971 indicate complex system. Component C occulted by Io revealed the 2.5 mag. fainter companion at 0.1".,DYN:0.004".,G:Sco OB2; Sco-Cen assoc.; probable member of Sco-Cen cluster; upper Sco region.,N:Graffias; Grafias; Grassias; Acrab; Akrab; Elacrab.,R:From occult. by Jupiter, diam. Beta Sco A1 = 0.000422"; diam. Beta Sco A2 = 0.000264".,S:Ca and Na lines nearly stationary.,SB:ADS 9913AD, 6.8281d, K 129.0k/s, V0 -1.0k/s, msin3i 16.0, asini 11.6. Mag. difference about 1v. Apsidal period,SB:51000 times orbital. Unresolved by speckle interferometry. Possible third SB component.
HR 5985	β²	8	BD-19 4308	144218	159683				9913 C	7424	16 05 26.5	-19 48 07	4.92	B2V	1.3	0.0	D:CPM with HR 5984, q.v.,G:Sco OB2; Sco-Cen assoc.; probable member of Sco-Cen cluster; upper Sco region.
HR 5988			CD-2312700	144334	184113					V929 Sco	16 06 06.3	-23 36 23	5.92	B8p v			G:Sco OB2; Sco-Cen cluster; member of the local association (Pleiades group); upper Sco region.,S:Helium-weak star.,VAR:Spectrum var., amp. 0.03V, 1.49187d.
HR 5993	ω¹	9	BD-20 4405	144470	184123						16 06 48.4	-20 40 09	3.96	B1V			G:Sco OB2; Sco-Cen cluster; member of the local association (Pleiades group); upper Sco region.
HR 5996			BD-13 4342	144585	159706						16 07 03.4	-14 04 15	6.32	G4IV-V
HR 5997	ω²	10	BD-20 4408	144608	184135		I			7454	16 07 24.3	-20 52 07	4.32	G3II-III			VAR:Amp. 0.02(b-y).
HR 5998			CD-2412552	144661	184142						16 07 51.9	-24 27 43	6.33	B7IIIp:			G:Sco OB2; Sco-Cen cluster; upper Sco region.,S:Helium-weak star.
HR 5999			CD-3810893	144668	207367			W	C	V856 Sco	16 08 34.2	-39 06 19	7.05	A7IVe	0.4	44.1	D:CPM with HR 6000 at 44". CD, 7.1, 11.7v, sep. 1.3".,VAR:6.97 - 7.71V, about 30d, variability attributed to circumstellar dust. Possibly a binary shell star with mass exchange.,VAR:Considerable confusion between HR 5999 and 6000 particularly as to which is the variable and which the brighter.,VAR:Originally announced as HR 6000, V856 Sco is really HR 5999, the southern preceding and fainter component C of the,VAR:bright double. The error stems from interchanged photometric data in Harvard Annals 45, 197, 1901, all other early,VAR:visual and photographic estimates indicating that the S. prec. component is the fainter.
HR 6000			CD-3810894	144667	207368			W	A		16 08 34.4	-39 05 35	6.65	A0-3III	0.4	44.1	D:CPM with HR 5999. Component B, 13v at 298".,S:Shell star.,VAR:Not the variable. Originally confused with HR 5999.
HR 6001			CD-2511369	144690	184144		I				16 08 07.6	-26 19 36	5.38	M2III
HR 6002		11	BD-12 4425	144708	159715				9924		16 07 36.4	-12 44 44	5.78	B9.5Vnn t	4.3	3.5	D:CPM.,S:Variable H alpha emission.
HR 6003			CD-2312731	144844	184164	3275				7470	16 08 43.7	-23 41 08	5.88	B9IVp:			G:Sco OB2; Sco-Cen cluster; upper Sco region.,RV:A recent determination of vsini =<15k/s.,S:Helium-weak star.
HR 6006			CD-3211456	144927	207396			W			16 09 31.7	-32 38 59	6.19	K0-2III	0.8	7.7	D:Components K0.5IIIab and F4III.
HR 6007			CD-3310961	144987	207403	3277					16 09 52.6	-33 32 45	5.54	B8V			G:Sco-Cen assoc.
HR 6012			BD-17 4502	145100	159745						16 09 55.2	-18 20 27	6.47	F4V
HR 6015			CD-4010251	145191	226564	3278					16 11 17.7	-41 07 11	5.86	F0IV			S:Also classified F2III + (A).
HR 6017			CD-2912343	145250	184197		I				16 11 02.0	-29 24 59	5.13	K3III
HR 6026	ν	14	BD-19 4332	145501	159763				9951 CD		16 11 58.6	-19 26 59	6.30	B8V+B9VpSi	2.5	41.1	D:ADS 9951 at least quintuple system with HR 6027 of which components CD = HR 6026 binary, 6.9 B8V or B9III, 7.9v B9Vp,,D:sep. 2". C is -19d4332.,DYN:0.009".,G:Sco OB2; Sco-Cen cluster; upper Sco member; reflection nebula and dust surrounding star. Assoc. Sco R1; IC 4592 at 145,G:pc.,RV:ADS 9951D, -3k/s; vsini 73k/s.,S:Also classified B9III+B9.5V.
HR 6027	ν	14	BD-19 4333	145502	159764				9951 AB		16 11 59.7	-19 27 38	4.01	B3V	2.5	41.1	D:ADS 9951A is SB, 4.9, 6.9v, sep. 0.0003". AB, binary. Component B, 6.9v at 1". Components CD at 41" = HR 6026, q.v.,D:HR 6026, q.v.,DYN:0.005".,G:Sco OB2; Sco-Cen assoc.; probable member of Sco-Cen cluster; upper Sco member; in reflection nebula, assoc. Sco R1; IC,G:4592 at 145 pc.,N:Jabbah.,S:H strong; SiIV weak for the spectral type.,SB:ADS 9951A 5.9222d, K 26.4k/s, V0 +1.4k/s, asini 2.15.
HR 6028		13	CD-2710841	145482	184221						16 12 18.2	-27 55 35	4.59	B2V			G:Sco OB2; Sco-Cen cluster? Upper Sco region; embedded in reflection nebulosity.
HR 6029		12	CD-2811962	145483	184217				9953	7520	16 12 15.9	-28 25 03	5.67	B9V v	2.1	3.9	D:Binary, companion F3V.,G:Sco OB2; upper Sco region.
HR 6031	ψ	15	BD-09 4324	145570	141022	3280					16 12 00.0	-10 03 51	4.94	A3IV			N:Some early catalogues (particlarly BAC) call Flamsteed 15 Chi instead of Psi Sco and leave 17 (HR 6048 =,N:Chi) unnumbered. All later sources adopt the convention followed here.
HR 6033		16	BD-08 4180	145607	141024						16 12 07.3	-08 32 51	5.43	A4V
HR 6042			CD-2412623	145792	184241				9967		16 13 45.7	-24 25 19	6.41	B5V	3.8	1.5	G:Sco OB2; Sco-Cen assoc.; upper Sco region; Sco-Cen cluster.
HR 6044			CD-3211525	145838	207480						16 14 22.3	-33 00 41	5.92	K0III
HR 6048	χ	17	BD-11 4096	145897	159793		I				16 13 50.9	-11 50 15	5.22	K3III			N:See HR 6031.
HR 6051			BD-20 4444	145964	184253						16 14 28.8	-21 06 27	6.41	A0V
HR 6053			BD-18 4249	145997	159807			D			16 14 39.1	-18 32 07	6.32	K2III	0.3	0.0	D:Sep. 0.03".
HR 6054			CD-2511453	146001	184258						16 14 53.6	-25 28 37	6.05	B7IV			G:Sco OB2; Sco-Cen cluster; upper Sco region.
HR 6060		18	BD-07 4242	146233	141066			W		7577	16 15 37.3	-08 22 10	5.50	G2Va	7.7	25.8	D:Optical.
HR 6061			BD-14 4383	146254	159821	3286				7578	16 15 51.5	-14 50 57	6.09	A0V
HR 6066			BD-20 4454	146416	184285						16 16 58.8	-21 18 14	6.61	B9V			G:Sco OB2; Sco-Cen cluster; upper Sco region.
HR 6070			CD-2812037	146624	184301	3288					16 18 17.9	-28 36 50	4.78	A0V
HR 6076			BD-19 4357	146834	184309						16 19 07.7	-20 13 04	6.29	K5III			C:UBV photometry indicates strong interstellar absorption, confirmed by neighboring stars. However, the spectral type is,C:considerably later than expected, even from the observed (B-V).,G:UMa stream; in reflection nebula; assoc. Sco R1. If a member of UMa stream, it must be an interloper in the upper Sco,G:nebulosities.,S:Variously classified G5III, G8IIIb, K0.5III and K5III.
HR 6077			CD-3013041	146836	207558	1426		W	A		16 19 32.7	-30 54 24	5.49	F6III	1.6	23.2	D:Companion, F9V, CPM.,SB:Component A of visual double.
HR 6078			BD-14 4398	146850	159846		I				16 19 00.4	-14 52 21	5.94	K4III
HR 6080			CD-3910412	146954	207574			W			16 20 32.6	-39 25 51	6.12	B9V	4.7	15.6
HR 6081	ο	19	CD-2312849	147084	184329		I			7632	16 20 38.2	-24 10 10	4.55	A5II v			C:Probably not IR source. Heavily reddened. Analysis of spectral energy distribution (Whittet 1988, MNRAS, 230, 473),C:shows no significant IR excess and possible overluminosity for A5II type.,G:Sco-Cen assoc.; upper Sco complex.,VAR:Small amp. in V. MgII 4481 appears to vary.
HR 6084	σ	20	CD-2511485	147165	184336	607	I		10009	Sig Sco	16 21 11.3	-25 35 34	2.89	B1III	2.0	0.0	C:Color excess E(B-V) = +0.40. Reddened star.,D:B, 8.26V, +0.25(B-V), -0.23(U-B), B9.5V at 20", optical; vsini : 54k/s. The visual primary is triple: SB, 3.3, 5.3v,,D:sep. 0.0005" and 5.5v at 0.49", discovered by occultation.,G:Sco OB2; Sco-Cen cluster; upper Sco region; HII region S9; in reflection nebula; assoc. Sco R1.,N:Alniyat; Al Niyat. Name applies to pair with HR 6165.,RV:ADS 10009B, -6k/s.,S:Stationary Ca lines. Although this star is an MK standard for class B1III, it is a variable, a multiple star, and is,S:situated in reflection nebulosity. Component A has also been classified as B2III and B2IV; component B as B9V, B9.5V,,S:and B8Vp. From scanner studies of composite spectra, Beavers (ApJS, 44, 489, 1980) finds ADS 10009A can be,S:resolved into O9.5 and B7 with a magnitude difference of 1.6V.,SB:ADS 10009A, 34.23d, K 34.0k/s, V0 +2.5k/s, asini 14.9.,VAR:Beta C 2.94 - 3.06B. Multiple periods, 0.2468429, 0.239671, 8.2, and 33.1d. Surrounded by HII region. Primary,VAR:period varies in period of 23.2y with an amp. of 0.7 sec. Occultations indicate the variable has a 2.2 mag. fainter,VAR:companion at 0".49. The duplicity had been suspected from occultations as early as 1860. Orbital period probably over,VAR:112 yrs. UV observations indicate temperature varies by 2510K and ratio max. to min. radius by 1.095.
HR 6094			CD-3810983	147513	207622	3295				7680	16 24 01.3	-39 11 35	5.40	G5V			VAR:Amp. 0.07V.
HR 6097			CD-3211687	147553	207625			W	A		16 23 56.7	-33 11 58	6.47	A0V+A0V	0.5	6.3	D:Components also classified B9.5V(n) and A1V(n).
HR 6100			CD-3710778	147628	207637			W			16 24 31.7	-37 33 57	5.42	B8IV	0.1	0.1	D:Sep. 0.098".,G:Sco-Cen assoc.
HR 6105			CD-2912513	147722	184368				10035 B		16 24 39.6	-29 42 12	6.63	G0IV	0.8	5.2	D:Binary with HR 6106, q.v.
HR 6106			CD-2912513	147723	184369				10035 A		16 24 39.7	-29 42 17	5.84	G0IV	0.8	5.2	D:Binary with HR 6105. Mag. and colors for combined light, 5.41V, +0.59(B-V), +0.12(U-B).
HR 6122			CD-3610783	148247	207688						16 28 14.7	-37 10 46	5.79	K1IIICNII
HR 6134	α	21	CD-2611359	148478	184415	616	I		10074	Alp Sco	16 29 24.4	-26 25 55	0.96	M1.5Iab-Ib+B4Ve	4.2	2.9	D:Var. M1Ib, 5.5 B2.5V, 878y, a = 2.90", masses 15.5 and 7.0 solar. Companion is radio source. SKYLAB confirms cool star,,D:hot companion.,DYN:0.011".,G:Sco OB2; Sco-Cen stream; in reflection nebula; assoc. Sco R1; dust shell beyond 12 R.,N:ANTARES; Cor Scorpii; Kalb al Akrab; Vespertilio.,R:Occultation diam. = 0.041".,RV:7.5 yrs.,S:Ultraviolet FeII emission. 5-micrometer observations indicate carbon monoxide.,VAR:ADS 10074A, SRc 0.88 - 1.8V, 1733d. Possibly considerably fainter before 150 A.D.: see HR 5685.
HR 6141		22	CD-2412695	148605	184429						16 30 12.4	-25 06 54	4.79	B2V			G:Sco OB2; probable member of Sco-Cen cluster, upper Sco region; in reflection nebula; assoc. Sco R1; IC 4605.
HR 6142			CD-4110695	148688	226855			W		7781	16 31 41.7	-41 49 01	5.33	B1Iae v	4.3	58.0	D:Components A (F5V) and B both optical.,S:Oxygen-rich supergiant.,VAR:Spectrum variable?
HR 6143			CD-3411044	148703	207732	1431					16 31 22.9	-34 42 16	4.23	B2III-IV			G:Sco-Cen cluster.
HR 6145			CD-2611379	148760	184437						16 31 22.8	-26 32 16	6.10	K1III
HR 6160			CD-4410964	149174	226926					7829	16 35 07.9	-45 14 41	6.46	K2-3III			VAR:Amp. 0.08V.
HR 6164			CD-4211399	149404	226953					V918 Sco	16 36 22.5	-42 51 32	5.47	O9Ia e			G:Ara OB1a. Listed by Buscombe and Kennedy (M.N.R.A.S. 124, 196, 1962) as among Sco-Cen stars. Buscombe now points out,G:that it is a nonmember background star.,RV:Two available determinations of vsini, 140 and 45k/s.,S:H alpha emission.,SB:9.813d, k1 101k/s, K2 60k/s, V1 -37k/s, V2 -28k/s, m1sin3i 1.6, m2sin3i 2.7,,SB:a1sini 13.7, a2sini 8.1.
HR 6165	τ	23	CD-2711015	149438	184481	620					16 35 53.0	-28 12 58	2.82	B0V			C:Color excess E(B-V) = +0.06.,G:Sco OB2; Sco-Cen cluster; Sco-Cen assoc.; upper Sco region. Faint HII region surrounds star. Member of Pleiades group.,N:See HR 6084.,S:Spectra indicate high velocity stellar wind. Lyman beta observed from COPERNICUS. High resolution UV spectrum,S:obtained from COPERNICUS. Large amount of atomic hydrogen, but only small amount of molecular hydrogen in line of sight.
HR 6166			CD-3411112	149447	207814		I			7844	16 36 22.5	-35 15 20	4.16	K6III
HR 6174			CD-4310959	149711	226989			W			16 38 26.2	-43 23 55	5.83	B2.5IV	3.2	16.3	D:CPM.,G:Member of the local association (Pleiades group); Sco-Cen assoc.
HR 6178			CD-3610879	149886	207878	3317		W			16 39 05.2	-37 13 03	5.91	B9-A0V+B	0.0	0.1	D:Sep. AB, 0.102".
HR 6192			CD-3211913	150331	207930						16 41 45.5	-33 08 47	5.87	G3III
HR 6206			CD-4010649	150573	227118			W			16 43 45.5	-41 07 08	6.20	A4V	0.1	95.7	D:CPM with HR 6209 at 96".,G:Sco OB1.
HR 6209			CD-4010653	150591	227123			W			16 43 53.9	-41 06 47	6.12	B6-7V	0.1	95.7	D:CPM with HR 6206.,G:Sco OB1.
HR 6210			CD-3710942	150608	207966			W			16 43 47.6	-38 09 24	6.05	B9II-III	6.2	50.0
HR 6211			CD-3113161	150638	207967	3325					16 43 38.7	-32 06 22	6.46	B8V
HR 6214			CD-4010661	150742	227146	3329		W			16 44 42.6	-40 50 23	5.71	B3V	6.3	8.	D:Secondary A5V, optical.,G:Member of the local association (Pleiades group); Sco OB1.
HR 6216			CD-2711103	150768	184591				10173	7935	16 44 17.3	-27 27 22	6.58	A2V	4.0	2.0	D:ADS 10173AB, binary.,VAR:E?, amp. 0.03V.
HR 6218			CD-2812358	150894	184602			W		7944	16 45 00.2	-28 30 35	6.02	A3IV	7.7	5.6
HR 6221			CD-3910677	151078	208020						16 46 47.8	-39 22 38	5.48	K0III
HR 6225		25	CD-2511667	151179	184630						16 46 51.3	-25 31 43	6.71	gG6
HR 6241	ε	26	CD-3411285	151680	208078	628				7983	16 50 09.8	-34 17 36	2.29	K2.5III
HR 6244			CD-3711023	151771	208089			W		Var?	16 50 59.8	-37 30 52	6.11	B9pSi*	2.2	6.7	RV:Companion -30k/s, double lines velocity separation 258k/s, both components B9V.,S:Also classified B8II/III.,VAR:Long per?
HR 6245			CD-4110957	151804	227313					7992	16 51 33.7	-41 13 50	5.22	O8Iaf			G:Sco OB1. Possible member of open cluster NGC 6231, 30' south of the center. See HR 6260.,RV:Outward moving atmosphere.,S:Shell star.
HR 6247	μ¹		CD-3711033	151890	208102	1439				Mu1 Sco	16 51 52.2	-38 02 51	3.08	B1.5V+B6.5V	0.4	390.	D:CPM with HR 6252 at 346".,G:Sco-Cen cluster; Sco-Cen assoc.; upper Sco; member of Pleiades group.,SB:1.4463d, K 185k/s, V0 0k/s, msin3i 9.09, asini 3.68. Equal components. Semi-detached system.,VAR:EB 2.80 - 3.08B, 1.44026907d. Semi-detached system.
HR 6249			CD-4110972	151932	227328		I			V919 Sco	16 52 19.1	-41 51 16	6.49	WN7-A			C:Strongly reddened.,G:Sco OB1; HII region; member NGC 6231. See HR 6260.,RV:3.5d not confirmed.,S:Circumstellar matter. Helium rich. The A in the spectral type here means narrow lines, not an A-type spectrum.,VAR:6.51 - 6.61V, HeI, NII 4097 var. 3.5d.
HR 6252	μ²		CD-3711037	151985	208116						16 52 20.1	-38 01 03	3.57	B2IV	0.4	390.	D:CPM with 6247 at 346".,G:Sco-Cen cluster; Sco-Cen assoc.; upper Sco; member of Pleiades group.
HR 6257			CD-4211627	152161	227359					8012	16 53 42.5	-43 03 03	5.96	M3II-III			VAR:Amp. 0.14V.
HR 6260			CD-4111024	152234	227377			W			16 54 01.8	-41 48 23	5.45	B0.5Ia	1.5	0.4	D:Component F, 7.3v O6, vsini 125k/s.,G:NGC 6231 #290. The open cluster NGC 6231 is the nucleus of Sco OB1 assoc., which is surrounded by an elliptical HII,G:region extending 4d or 5d. Diam. of cluster 26'. Considerable dark nebulosity close to cluster. HR 6245, 6249, 6261 and,G:6265 also in the cluster.,S:Nitrogen deficient.
HR 6261			CD-4111021	152235	227374					V900 Sco	16 53 58.8	-41 59 41	6.32	B1Ia e			C:Strongly reddened.,G:Sco OB1; in cluster NGC 6231. See HR 6260.,S:H alpha emission. Nitrogen deficient. Strong OII.,VAR:6.29 - 6.34V, 2.631? or 6.28 or 6.85d.
HR 6262	ζ¹		CD-4211633	152236	227375					Zet1 Sco	16 53 59.7	-42 21 44	4.73	B1Iape v			C:Strongly reddened.,G:Possible member of NGC 6231, 30' south of the center of the cluster. See HR 6260.,RV:Mass loss estimated 0.00005 solar masses/y.,S:Shell star. Possible H alpha emission.,VAR:Amp. 0.09V. Variations in HeI, NII, OII suggest turbulent outer layers.
HR 6263			CD-4111036	152249	227383					8023	16 54 11.8	-41 51 01	6.45	O9Ib			G:Sco OB1; in open cluster NGC 6231 #293. See HR 6260.,S:Also classified OC9.5Iab, OC9.5I and O9.5I.,SB:5.97d, K1 191k/s, K2 206k/s, V1 -44k/s, V2 -8k/s, msin3i 20.1, asini 15.7.,VAR:6.34 - 6.50V.
HR 6265			CD-4111041	152270	227390			W		Var?	16 54 19.6	-41 49 12	6.59	WC7+O5-8	6.6	4.3	C:Strongly reddened.,D:Innes and IDS data on components and number of components appear inconsistent. Probably different cluster components,D:measured.,G:In cluster NGC 6231 #220. See HR 6260.,RV:Shell of WR component expanding at 1688k/s.,SB:Component A of visual double, 8.893d, K 142k/s, V0 -27.2k/s, msin3i 1.75, asini 17.4. Same period for both,SB:absorption and emission lines, but differ in phase by 0.5 period.
HR 6266			CD-4211642	152293	227392						16 54 26.9	-42 28 44	5.88	F5Ib-II			G:Sco OB1.
HR 6271	ζ²		CD-4211646	152334	227402					8028	16 54 35.0	-42 21 41	3.62	K4III			G:Sco OB1.,VAR:3.6 - 3.64V.
HR 6272			CD-4010919	152408	227425			W		8031	16 54 58.4	-41 09 04	5.77	O8:Iafpe	7.0	5.4	D:Companion F4p.,G:Runaway star from Sco OB1. Possible member NGC 6231, 30' south of the center of the cluster. See HR 6260.,M:Either runaway, or P Cyg type with extended expanding atmosphere.,RV:Mass loss 0.00009 solar masses/y.,S:Shell star. Sp. shows interstellar Lambda4430.,VAR:Amp. 0.07V.
HR 6273			CD-3013594	152431	208176						16 54 36.0	-30 35 14	6.35	A7IIIm:
HR 6282			CD-3311570	152636	208205						16 55 57.8	-33 30 26	6.37	K5III
HR 6283			CD-4010975	152667	227473					V861 Sco	16 56 36.0	-40 49 25	6.15	B0.5Ia e			C:Strongly reddened.,G:In cluster Collinder 316; Sco OB1.,RV:Also 0.6147d related to rotation of primary. Mass loss 0.000027 solar masses/y.,S:H alpha emission. Nitrogen deficient. P Cyg type?,SB:7.8483d, K 84.5k/s, V0 -34.6k/s, asini 9.09. Alternate orbits 7.8483d, K 99.4k/s, V0 -43.3k/s; 7.848250d,,SB:K 82k/s, V0 -31k/s; 7.84825d, K 87.3k/s, V0 -34.4k/s, asini 9.4. Low mass companion. Tidal distortion.,VAR:EB 6.07 - 6.69V, 7.84818d.
HR 6288		27	CD-3311590	152820	208232						16 57 11.1	-33 15 34	5.48	K5III
HR 6298			CD-3711131	153072	208259			W			16 58 52.4	-37 37 16	6.09	A3V	0.2	0.2	D:6.7 A3V, 6.9 A4V, 37.9y, a = 0.181". Combined mag., colors.
HR 6303			CD-4511123	153258	227547						17 00 32.3	-45 27 06	6.65	K4III
HR 6311			CD-3511236	153368	208293						17 00 36.9	-35 56 03	5.97	K2IIICNII
HR 6316			CD-3113473	153613	208324	3354		W			17 01 52.7	-32 08 37	5.03	B8V	7.5	23.8	D:All companions optical. B is A8V, C is F5V.,G:Sco-Cen assoc.
HR 6327			CD-3711201	153890	208355					V923 Sco	17 03 50.8	-38 09 08	5.91	F4IV+F2V			G:NGC 6281 #1 (nonmember).,SB:34.8189d, K 53.6k/s, V0 -14.8k/s, msin3i 1.48, asini 23.3.,VAR:E amp. 0.35V, 34.8269:d.
HR 6331			CD-4511188	154025	227601						17 05 05.3	-45 30 06	6.28	A2V
HR 6334			CD-3311706	154090	208377			W			17 04 49.4	-34 07 22	4.87	B1Ia t	9.1	20.	G:Sco-Cen assoc.; doubtful member of the Sco-Cen cluster.,VAR:H alpha profile variable.
HR 6338			CD-4311396	154153	227615						17 05 48.6	-44 06 18	6.19	A4III
HR 6344			CD-3711274	154310	208406			W			17 06 20.3	-37 13 39	5.98	A2IV	4.9	5.8
HR 6347			CD-3511306	154368	208410			W			17 06 28.4	-35 27 04	6.13	O9.5Iab	6.5	2.8	C:B-V values scatter from +0.38 to +0.60, U-B from -0.37 to -0.63.,G:Sco OB4. Listed by Buscombe and Kennedy (M.N.R.A.S. 124, 196, 1962) as among Sco-Cen stars. Buscombe now points out,G:that it is a nonmember background star.,S:Strong interstellar lines indicate the interstellar molecules CH, CH+, and CN are in localized area near the Sun.
HR 6366			CD-3013840	154783	208467	3363					17 08 47.5	-30 24 13	5.97	A/FmDel Del			G:Hyades group.,S:Also classified F0III.
HR 6371			CD-4411502	154948	227688			W			17 10 42.3	-44 33 27	5.08	G8-K0III+G	7.9	13.2
HR 6380	η		CD-4311485	155203	227707	638					17 12 09.2	-43 14 21	3.33	F3III-IVp			G:Hyades group.,S:Also classified F2V.
HR 6381			CD-3911182	155259	208521	3366					17 12 16.2	-39 30 25	5.67	A1V
HR 6382			CD-3811632	155276	208522						17 12 16.5	-38 49 20	6.30	K1IIICNII
HR 6389			CD-3212460	155450	208539			W			17 12 58.7	-32 26 19	6.01	B1II	7.5	30.	G:Sco OB4; doubtful member of the Sco-Cen cluster; possible new OB assoc. in Sco with HR 6397 and HR 6422.
HR 6392			CD-3911212	155603	208569		I	W		V915 Sco	17 14 27.7	-39 46 01	6.60	G5Ia	4.2	14.4	D:Component B, 10.42V, +0.52(B-V); component C, 11.40V, +1.55(B-V).,VAR:Amp. 0.15V.
HR 6397			CD-3311875	155806	208585					8388	17 15 19.3	-33 32 54	5.53	O7.5V[n]e			G:Sco OB4 assoc.; possible new OB assoc. in Sco with HR 6389 and HR 6422.,S:Variously classified O5pe, O7.5-O8IIIe, O7.5Vne, O8-O9Ve.,VAR:Emission lines variable? H alpha width and profile vary.
HR 6398			CD-3811686	155826	208591			W			17 15 35.9	-38 35 38	5.96	F7V+G2V	0.1	0.1	D:Sep. 0.108". Speckle observations 1986.45 give 0.14".
HR 6403			CD-3013968	155940	208606						17 15 51.5	-30 12 38	6.21	B9.5V
HR 6405			CD-3511426	155974	208610			W			17 16 21.5	-35 44 58	6.12	G0IV-V	7.4	36.5
HR 6409			CD-3212545	156098	208626	1452					17 17 03.7	-32 39 46	5.55	F6IV			G:Hyades group.
HR 6420			CD-4311572	156293	227813						17 18 48.0	-44 07 47	5.76	B9V
HR 6422			CD-3212573	156325	208657			W		Var?	17 18 20.4	-32 33 12	6.36	B5Vn e	5.6	19.5	D:Companion is F2V.,G:Sco OB4; Sco-Cen assoc. See HR 6389.,VAR:Amp. 0.04V on time scale 3 hrs. and 0.05 on time scale 1d suspected.
HR 6426			CD-3411626	156384	208670			W		8482	17 18 57.2	-34 59 23	5.91	K3V+K5V	1.0	0.5	D:AB 6.1 K3V, 7.6 K5V, 42.177y, a = 1.734" or 42.09y, a = 1.82", combined mag., colors. Component C, 9.9v M2, 32",D:physical. D, 12.8v at 15".,DYN:0.144".,VAR:Amp. 0.04.
HR 6427			CD-4411595	156398	227821			W			17 19 24.5	-44 13 23	6.65	B9.5V+A6III	0.3	0.2	D:Binary. Combined mag., colors, sep. 0.200".
HR 6450			CD-3711507	157038	208740			W			17 22 39.4	-37 48 18	6.41	B4Ia	5.8	2.7	C:V magnitudes scatter from 6.31 to 6.44, B-V from +0.61 to +0.89, U-B from +0.01 to -0.30.,G:Sco-Cen assoc.; in HII region.,S:NII and MgII indicate different spectral classes. Component B is G type.
HR 6454			CD-3511505	157060	208741						17 22 38.0	-35 54 36	6.47	F7V
HR 6456			CD-3711512	157097	208747			W			17 22 54.9	-37 13 14	5.93	K1III	8.4	20.2
HR 6460			CD-4411669	157243	227911						17 24 13.0	-44 09 45	5.12	B7III			G:Sco-Cen assoc.
HR 6470			CD-3411674	157486	208786						17 25 02.7	-34 41 47	6.16	A0VSiCr
HR 6501			CD-3611546	158105	208860						17 28 56.1	-36 46 42	6.02	K0III
HR 6503			CD-3811927	158156	208870			W			17 29 25.7	-38 31 00	6.39	A2V	0.3	0.4
HR 6508	υ	34	CD-3711638	158408	208896	649					17 30 45.8	-37 17 45	2.69	B2IV			C:Color excess E(B-V) = +0.02.,G:Sco-Cen assoc.,N:Lesath; Lesuth.,S:Lyman alpha and Lyman beta observed from COPERNICUS.
HR 6517			CD-3312149	158619	208921						17 31 47.4	-33 42 10	6.44	K2III
HR 6522			CD-3411757	158741	208935					V949 Sco	17 32 24.5	-34 16 47	6.17	F2V
HR 6523			CD-4111742	158799	228110						17 33 07.4	-41 10 25	5.84	B9Ib-II
HR 6527	λ	35	CD-3711673	158926	208954	652		W		Lam Sco	17 33 36.5	-37 06 14	1.63	B2IV+B	10.3	94.9	C:Color excess E(B-V) = +0.03.,G:Sco-Cen assoc.,N:SHAULA.,S:Lyman alpha and Lyman beta observed from COPERNICUS.,SB:5.6d. Interferometer measures indicate multiple star.,VAR:Beta C 1.59 - 1.65V, 0.2137015d, secondary 0.1068518d, beat period 10.1605d. Also possible 0.04V eclipse. X-ray,VAR:flare observed in vicinity Lambda Sco on 1 June 1975.
HR 6535			CD-3212935	159176	208977			W		9167	17 34 42.5	-32 34 54	5.70	O7V+O7V	4.8	5.4	D:Component B, B9V; C, B8V.,G:In cluster NGC 6383 #1; in HII reg. Ma 322; in nebulosity. Embedded in large neutral hydrogen complex of which a small,G:part is ionized by the hot O7-type star.,M:Central star of open cluster NGC 6383, probably older than the rest of the cluster core and might have initiated star,M:formation in the core and beyond.,SB:3.3666d, K 213.8k/s, V0 +9.1k/s, msin3i 12.7, asini 9.90. Two O7V components, about 30 solar masses. vsini of,SB:secondary 148k/s.,VAR:Ell?, 5.68 - 5.71V.
HR 6539			CD-3711702	159312	209001						17 35 43.0	-37 26 24	6.48	A0V
HR 6546			CD-3812044	159433	209019					9205	17 36 32.8	-38 38 07	4.29	K0IIIb
HR 6553	θ		CD-4212312	159532	228201	654				9233	17 37 19.2	-42 59 52	1.87	F1II			N:Sargas.,VAR:1.90 - 1.94V?
HR 6557			CD-3711723	159633	209034						17 37 26.8	-38 03 56	6.26	G2Ib
HR 6558			CD-4212327	159707	228220						17 38 08.5	-42 52 50	6.10	B8V
HR 6580	κ		CD-3812137	160578	209163	660				Kap Sco	17 42 29.3	-39 01 48	2.41	B1.5III			G:Sco-Cen assoc.,SB:Same periods as VAR.,VAR:Beta C 2.39 - 2.42V, 0.1998303d, 0.205430, 7.3316, 0.189512 and 2.591d.
HR 6583			CD-3611804	160668	209172						17 42 51.0	-36 56 45	5.54	K5III
HR 6587			CD-3213208	160748	209176						17 43 06.9	-33 03 04	6.40	M1III
HR 6597			CD-4212431	160928	228363			W			17 44 42.0	-42 43 44	5.87	A1V+F0IV	0.1	0.1	D:Sep. 0.111".
HR 6613			CD-3812189	161390	209246			W			17 47 07.3	-38 06 42	6.43	B9V+A1V	0.3	0.1	D:7.1 B9, 7.3, 34.00y, a = 0.157". Combined mag., color.
HR 6615	ι¹		CD-4011838	161471	228420	666		W			17 47 35.1	-40 07 37	3.03	F2Iae	9.9	37.5
HR 6628			CD-3114609	161840	209303						17 49 10.5	-31 42 12	4.83	B8V
HR 6630			CD-3711907	161892	209318	669		W			17 49 51.5	-37 02 36	3.21	K2III	11.5	41.7
HR 6631	ι²		CD-4011886	161912	228466			W			17 50 11.2	-40 05 26	4.81	A2Ib	6.1	32.6
HR 6643			CD-4011905	162189	228489			W			17 51 32.8	-40 46 21	5.96	M2III	6.5	23.6
HR 6645			CD-3014802	162220	209357			W			17 51 12.5	-30 33 26	6.66	A0Vn	1.5	10.2	D:Companion A0IV. Fixed sep.
HR 6647			CD-3412165	162374	209383					V957 Sco	17 52 13.6	-34 47 57	5.90	B6V v			G:Open cluster NGC 6475 #26; M7 blue straggler.,RV:He lines show var. RV; H, Mg, Si do not.,VAR:SX Ari, amp. 0.05V, 1.658d. Spectrum variable.
HR 6648			CD-3412170	162391	209390						17 52 19.7	-34 25 00	5.84	G8III
HR 6649			CD-4112139	162396	228510						17 52 52.7	-41 59 48	6.20	F8IV-V
HR 6651			CD-3412186	162496	209397						17 52 49.2	-34 06 51	6.06	K1III
HR 6652			CD-3412187	162515	209401						17 52 55.9	-35 01 07	6.45	B9.5V			G:Open cluster NGC 6475 #42; M7.,SB:6.67683d, K 57.6k/s, V0 -8.7k/s, asini 5.29. Alternate orbit 6.6768d, K 53.4k/s, V0 -12.3k/s, asini 4.90.,SB:Secondary much fainter.
HR 6653			CD-3512013	162517	209404						17 52 57.9	-35 37 27	6.03	F2III-IV
HR 6657			CD-3412200	162586	209411			W			17 53 19.6	-34 43 50	6.17	B8V	0.0	0.1	D:6.9, 6.9v, 160.759y, a = 0.37".,G:Open cluster NGC 6475 #56.
HR 6658			CD-3412203	162587	209416			W			17 53 23.3	-34 53 43	5.60	K3III	0.1	0.4	D:Binary.,G:Open cluster NGC 6475 #58.
HR 6660			CD-3412219	162678	209425						17 53 45.5	-34 47 09	6.38	B9V			G:NGC 6475 #141.
HR 6662			CD-3412226	162724	209428			W		V906 Sco	17 53 54.9	-34 45 09	5.96	B9V+B9V	0.8	0.3	G:Sco-Cen assoc.; open cluster NGC 6475 #86.,SB:2.7754d, K 121k/s, V0 -32k/s, msin3i 3.15, asini 4.54. Triple-lined SB. vsini of secondary 50k/s.,VAR:E? Amp. 0.26V.
HR 6663			CD-3412228	162725	209430					V951 Sco	17 53 58.1	-34 49 54	6.42	ApSi*			G:Open cluster NGC 6475 #88.,S:Also classified A0VpSiCr, B9Si, and B9III.,VAR:Amp. 0.04V. Possible periods 4.45597, 4.4588d (North 1984, A&AS, 55, 259).
HR 6668			CD-3412244	162817	209446						17 54 27.2	-34 27 59	5.96	B9.5V			G:NGC 6475 #110.
HR 6671			CD-3612008	162926	209458						17 55 07.9	-36 28 33	6.06	B9.5III
HR 6675			CD-4412201	163145	228562	3425					17 56 47.4	-44 20 32	4.86	K2III
HR 6678			CD-4012001	163234	228564						17 56 55.8	-40 18 20	6.43	K3III
HR 6682			CD-4112231	163376	228578						17 57 47.7	-41 42 58	4.88	M0III
HR 6683			CD-3912058	163433	209524			W			17 57 57.8	-39 08 13	6.29	A0IV-V	1.5	0.7

Revised+Historic NGC/IC, Version 22/9, © Dr. Wolfgang Steinicke ^[277]
Planetary Nebulae
Name	RA	Dec	Type	bMag	vMag	Dim	Dreyer Description	Identification, Remarks
NGC 6072	16 12 58.2	-36 13 46	PN	14.1	11.7	1.63	pF, R, vgvlbM, r	PK 342+10.1, ESO 389-PN15, AM 1609-360, CS=17.5
NGC 6153	16 31 30.6	-40 15 11	PN	11.5	10.9	0.4	planetary, stellar	PK 341+5.1, ESO 331-PN6, AM 1628-400
NGC 6302	17 13 44.1	-37 06 12	PN	12.8	9.6	1.48	pB, E pf (Swift: triple)	PK 349+1.1, ESO 392-PN5, Sh2-6, Bug nebula
NGC 6337	17 22 15.7	-38 28 59	PN	11.9	12.3	0.85	!!! annular, eF, S, am st	PK 349-1.1, ESO 333-PN5, AM 1718-382, CS=14.8
IC 4599	16 19 23.2	-42 15 34	PN	12.4		0.25	Planetary, 15 mag	PK 338+5.1, ESO 331-PN1, AM 1615-420
IC 4637	17 05 10.4	-40 53 05	PN	13.6	12.5	0.37	Planetary, stellar	PK 345+0.1, ESO 332-PN21, CS=12.3
IC 4663	17 45 28.7	-44 54 16	PN	13.1	12.5	0.33	Planetary, stell	PK 346-8.1, ESO 279-PN6, CS=14.0
Galactic Nebulae
Name	RA	Dec	Type	bMag	vMag	Dim	Dreyer Description	Identification, Remarks
NGC 6334	17 20 48.0	-36 06 12	EN			35 × 20	cF, vL, icE, vglbf, * 8 inv	ESO 392-EN9, Sh2-8, CED 140
NGC 6357	17 24 43.5	-34 12 05	EN+OCL			25 × 25	F, L, E, vglbM, D * inv	ESO 392-SC10, CED 142, Sh2-11
IC 4591	16 12 18.0	-27 55 40	RN+*			12 × 10	* 5.6 in F neb	LBN 1096, ESO 451-*N16
IC 4592	16 11 59.6	-19 27 35	RN+*			150 × 60	vL, E, ν2 Scorpii inv	LBN 1113, ESO 584-N*6, CED 128
IC 4601	16 20 18.0	-20 04 54	RN+*			20 × 10	2 st 8 in eL, dif neb, lE npsf	ESO 585-*N1, CED 129C
IC 4605	16 30 12.5	-25 06 53	RN+*			30 × 30	* 7 in eF, vL neb	LBN 1110, ESO 517-*N8, CED 133
IC 4628	16 57 00.0	-40 27 24	EN			90 × 60	F, eL, E pf, dif	ESO 332-EN14
Open Clusters
Name	RA	Dec	Type	bMag	vMag	Dim	Dreyer Description	Identification, Remarks
NGC 6124	16 25 17.2	-40 40 01	II3m		5.8	40	Cl, B, L, pRi, lCM, st 9…11	OCL 990, ESO 331-SC3
NGC 6178	16 35 50.8	-45 38 48	I3p		7.2	5	Cl, B, S, st pL	OCL 980, ESO 276-SC6
NGC 6192	16 40 20.8	-43 21 55	I2p		8.5	9	Cl, pL, pRi, iR, st 11…14	OCL 988, ESO 277-SC3
NGC 6216	16 49 23.5	-44 43 53	II2p		10.1	4	Cl, pS, pRi, pC, st 12…15	OCL 989, ESO 277-SC14
NGC 6231	16 54 09.8	-41 49 30	I3p	2.8	2.6	14	Cl, B, cL, pRi, st 10…13	OCL 997, ESO 332-SC6
NGC 6242	16 55 30.6	-39 28 01	I3m		6.4	9	Cl, B, L, Ri, st 8…11	OCL 1001, ESO 332-SC10
NGC 6249	16 57 41.7	-44 48 17	II1p		8.2	6	Cl, pRi, vlC, iF, st L & S	OCL 994, ESO 277-SC19
NGC 6259	17 00 45.3	-44 39 18	III2m		8.0	15	! Cl, B, vL, vRi, st 11…	NGC 6222, OCL 996, ESO 277-SC22
NGC 6268	17 02 04.1	-39 43 16	II2p		9.5	6	Cl, B, pL, cRi, st 10…	OCL 1002, ESO 332-SC17
NGC 6281	17 04 47.2	-37 53 16	II2p		5.4	8	Cl, L, pRi, lC, st 9…11	OCL 1003, ESO 332-SC19
NGC 6318	17 16 13.4	-39 25 26	III2p		11.8	5	Cl, pL, Ri, R, gbM, st 12…14	OCL 1004, ESO 333-SC1
NGC 6322	17 18 25.7	-42 56 02	I2p		6.0	5	Cl, vL, pRi, lC (place of * nf)	OCL 1000, ESO 278-SC6
NGC 6383	17 34 42.2	-32 34 54	IV3p	5.6	5.5	20	Cl, st 13, * 6·7 in M	NGC 6374, OCL 1026, ESO 393-SC7
NGC 6396	17 37 36.2	-35 01 33	II3p		8.5	3	Cl, pL, lRi, lC	OCL 1018, ESO 393-SC10
NGC 6400	17 40 12.0	-36 57 42	II2m		8.8	12	Cl, pL, pRi, iR, st 9…10	OCL 1014, ESO 393-SC14
NGC 6404	17 39 37.3	-33 14 48	III3m		10.6	6	Cl, F, L, pRi, lC, st 13…15	OCL 1024, ESO 393-SC13
NGC 6405	17 40 20.0	-32 15 30	III2p	4.5	4.2	33	Cl, L, iR, lC, st 7, 10…	M 6, OCL 1030, ESO 455-SC30, Butterfly cluster
NGC 6416	17 44 19.9	-32 21 40	IV1p		5.7	15	Cl, vL, Ri, lC	OCL 1031, ESO 455-SC32
NGC 6425	17 47 00.0	-31 31 48	I1p		7.2	10	Cl, pS, lRi, lC, st 10…12	OCL 1033, ESO 455-SC38
NGC 6444	17 49 35.1	-34 49 11	III2m			12	Cl, vL, vRi, st 12…13	OCL 1023, ESO 393-SC30
NGC 6451	17 50 40.5	-30 12 42	II1p		8.2	8	Cl, pL, pRi, bifid, st 12…	OCL 1035, ESO 455-SC50
NGC 6475	17 53 50.0	-34 47 36	II2r	3.5	3.3	75	Cl, vB, pRi, lC, st 7…12	M 7, OCL 1028, ESO 394-SC9, Ptolemy's cluster
Globular Clusters
Name	RA	Dec	Type	bMag	vMag	Dim	Dreyer Description	Identification, Remarks
NGC 6093	16 17 02.5	-22 58 28	II		7.3	10	!! globular, vB, L, vmbM (var *), rrr, st 14	M 80, GCL 39, ESO 516-SC11
NGC 6121	16 23 35.5	-26 31 29	IX		5.4	36	Cl, 8 or 10 B st in line, with 5 st, rrr	M 4, GCL 41, ESO 517-SC1
NGC 6139	16 27 40.4	-38 50 54	II		9.1	8.2	B, pL, R, psbM, rr	GCL 43, ESO 331-SC4
NGC 6144	16 27 14.1	-26 01 27	XI		9.0	7.4	Cl, cL, mC, gbM, rrr	IC 4606, GCL 42, ESO 517-SC6
NGC 6256	16 59 32.6	-37 07 15	GCL		11.3	4.1	globular, vF, vL, iR, vgbM, rrr	GCL 49.1, ESO 391-SC6, vdB-Hagen 208
NGC 6380	17 34 28.0	-39 04 07	GCL		11.5	3.6	eF, pS, lE, * 9 att	GCL 68, ESO 333-SC14
NGC 6388	17 36 17.0	-44 44 04	III		6.8	10.4	globular, vB, L, R, pg, psvmbM, rrr, st 17…	GCL 70, ESO 279-SC2
NGC 6441	17 50 12.9	-37 03 02	III		7.2	9.6	globular, vB, pL, R, vgmbM, rrr, st 18	GCL 78, ESO 393-SC34
NGC 6453	17 50 51.8	-34 35 53	IV		10.2	7.6	cL, iR, pmbM, r	GCL 79, ESO 393-SC36
NGC 6496	17 59 02.0	-44 15 52	XII		8.6	5.6	Neb + Cl, pL, mE, gvlbM	GCL 80, ESO 279-SC13
Galaxies
Name	RA	Dec	Type	bMag	vMag	Dim	Dreyer Description	Identification, Remarks
NGC 6000	15 49 49.4	-29 23 13	SBbc	12.7	11.9	1.9 × 1.6	vF, S, R, sbM	ESO 450-20, MCG -5-37-3, IRAS 15467-2914
IC 4596	16 16 03.6	-22 37 29	SBab	14.8	14.0	1.5 × 0.5	F, S, mE 40°, mbMN, prob spir	ESO 516-9, MCG -4-38-5
IC 4597	16 17 39.7	-34 21 58	S0-a	14.6	13.7	1.2 × 1	bM, magn 14	ESO 380-2, IRAS 16144-3414
IC 4598	16 18 13.2	-31 26 29	Sbc	14.6	13.8	1.5 × 0.4	Neb streak of F st, 1' ns	ESO 451-18, IRAS 16150-3119
IC 4600	16 16 05.3	-22 46 59	S0-a	16.4	15.5	0.4 × 0.4	eF, eS, R	ESO 516-10

«Strasbourg-ESO Catalogue of Galactic Planetary Nebulae» Acker et al., 1992 ^[141]
PNG	RA	Dec	Main ID	PK	IRAS	Discoverer	Identities	oDiam ["]	rDiam ["]	Dist [kpc]	Rvel [km/s]	ExpVel [km/s]	C* Name	C* Mag	C* SP Type
PN G000.3-02.8	17 57 42	-30 02 02	M 3-47	0-02.5		MINKOWSKI 1948	ESO 456-22, Sa 3-100, VV' 296	0.			-16.0 ± 5.0
PN G000.5-03.1	17 59 16	-30 02 48	KFL 1			KINMAN et al 1988		8.2			-51.0			B: 18.4, V: 17.3
PN G338.8+05.6	16 19 23	-42 15 36	He 2-155	338+05.1	16158-4208	HENIZE 1964	Sa 2-141, ESO 331-01, Wray 16- 215	14.5			-26.5 ± 8.8			B: 16.7, V: 16.3
PN G341.8+05.4	16 31 31	-40 15 22	NGC 6153	341+05.1	16280-4008	COPELAND 1883	ARO 501, ESO 331-06, He 2- 167, RCW 112, Sa 2- 148, VV 81, VV' 141, Wray 16-225	24.		1.8	+37.0 ± 3.0	17.5 (O-III), 17. (N-II)	AG82 210bis, CD -39 10464, GCRV 9495, HD 148687	B: 16.14
PN G342.1+10.8	16 12 59	-36 13 39	NGC 6072	342+10.1	16097-3606	HUBBLE 1921	ARO 500, ESO 389-15, My 93, Sa 2- 134, VV 77	70.		1.9	+7.0 ± 2.0	< 6.0 (O-III), 10.0 (N-II)	AG82 200	B: 19.31
PN G342.7+00.7	16 53 31	-42 39 18	H 1- 3	342+00.1		HARO 1952	ESO 277-17, Sa 3- 38, VV' 146, Wray 16- 239	16.
PN G342.9-02.0	17 06 23	-44 13 12	Pe 1- 8	342-02.1	17027-4409	HENIZE 1964	ESO 278-03, He 2- 198, Sa 2-173, VV' 159, Wray 16- 249	19.			-1.0 ± 3.0	26.9 (O-III)
PN G343.0-01.7	17 05 39	-43 57 27	Vd 1-9	343-01.1	17020-4352	VANDERVORT 1964	ESO 278-01	0.
PN G343.3-00.6	17 01 28	-43 05 56	HaTr 5			HARTL et al 1983		120.						B: 17.8, V: 16.4
PN G343.4+11.9	16 13 28	-34 35 42	H 1- 1	343+11.1		HARO 1952	ESO 389-16, Sa 2-135, StWr 4- 5, VV' 134, Wray 16- 209	2.4					AG82 201, HARO 1- 1	B: 16.87, V: 17.30
PN G343.6+03.7	16 44 24	-40 03 20	SuWt 3			SCHUSTER et al 1980		20.			-194.0 ± 15.0		AG82 213	B: 20.5, V: 20.5
PN G343.9+00.8	16 57 24	-41 37 56	H 1- 5	344+00.1	16538-4133	HARO 1952	ESO 332-15, Sa 3- 39, VV' 149, Wray 16- 243	5.2
PN G344.2+04.7	16 42 33	-38 54 27	Vd 1-1	344+04.1	16391-3848	VANDERVORT 1964	ESO 331-08, He 2- 178, Sa 2-151, Wray 16- 231	0.			-142.1 ± 3.5			B: 16.9, V: 16.7
PN G344.2-01.2	17 07 00	-42 41 15	H 1- 6	344-01.1		HARO 1952	ESO 278-04, He 2- 199, Sa 3- 40, VV' 160, Wray 16- 250	12.
PN G344.4+02.8	16 50 33	-40 03 00	Vd 1-5	344+02.1		VANDERVORT 1964	ESO 332-04, Sa 2-156	0.
PN G344.4-06.1	17 30 04	-45 22 50	Wray 16-278			WRAY 1966	Sa 2-208	0.
PN G344.8+03.4	16 49 33	-39 21 10	Vd 1-3	344+03.1		VANDERVORT 1964	ESO 332-02, Sa 3- 37	0.
PN G345.0+03.4	16 50 25	-39 08 19	Vd 1-4	345+03.1	16469-3903	VANDERVORT 1964	ESO 332-03, He 3-1261, Sa 2-154, Wray 16- 235	5. :
PN G345.0+04.3	16 46 45	-38 36 58	Vd 1-2	345+04.1	16433-3831	VANDERVORT 1964	ESO 332-01	0.
PN G345.0-04.9	17 26 12	-44 11 29	Cn 1-3	345-04.1	17225-4408	CANNON 1921	ESO 278-09, He 2- 220, PC 15, Sa 2-195, StWr 2-30, Wray 16- 272	< 5.			-78.0 ± 5.0			B: 14.6, V: 14.3
PN G345.2-01.2	17 10 27	-41 52 49	H 1- 7	345-01.1	17069-4149	HARO 1952	AS 219, ESO 332-24, He 2- 200, Sa 2-174, VV' 164, Wray 16- 254	8.5					AG82 231
PN G345.4+00.1	17 05 09	-40 52 57	IC 4637	345+00.1		FLEMING 1901	ESO 332-21, He 2- 193, Sa 2-168, VV 89, VV' 156, Wray 15-1607	18.5		1.5	+11.2 ± 4.9	21.0 (O-III)	AG82 224, CD -40 11127, CPD -40 7710, GCRV 9841, HD 154072	B: 12.88, V: 12.50	O(H)
PN G345.6+06.7	16 39 28	-36 34 22	He 2-175	345+06.1	16361-3628	HENIZE 1964	ESO 391-01, Sa 2-150, Wray 16- 229	6.6			-32.0 ± 5.0
PN G345.9+03.0	16 54 27	-38 44 08	Vd 1-6	345+03.2	16510-3839	VANDERVORT 1964	ESO 332-07, Sa 2- 159, Wray 16- 241	20. :
PN G346.0+08.5	16 34 04	-35 05 26	He 2-171	346+08.1	16307-3459	HENIZE 1964	ESO 390-07, Wray 16- 226	< 10.			-83.0 ± 25.0
PN G346.2-08.2	17 45 29	-44 54 11	IC 4663	346-08.1	17417-4453	FLEMING 1901	ESO 279-06, He 2- 273, Sa 2- 236, StWr 2- 32, VV 111, VV' 239, Wray 16- 303	13.			-48.7 ± 9.0	15.0 (O-III)	AG82 256, CSI -44 -17417, HD 161028	B: 16.0, V: 15.2	IUE obsns
PN G346.3-06.8	17 39 20	-44 09 38	Fg 2	346-06.1	17356-4408	FLEMING 1909	ESO 279-04, He 2- 257, Sa 2-225, StWr 2-31, VV 106, VV' 224, Wray 16- 293	< 5.			+35.0 ± 4.0
PN G346.9+12.4	16 23 17	-31 44 57	K 1- 3	346+12.1		KOHOUTEK 1962	A 38, ESO 452-01, Wray 19- 45	92.			-12.8 ± 6.0	17.0 (O-III)	AG82 207	B: 20.5
PN G347.4+05.8	16 48 53	-35 47 13	H 1- 2	347+05.1	16456-3542	HARO 1952	AS 208, ESO 391- 03, He 2- 181, MHa 300- 58, Sa 2-153, VV' 144, Wray 16- 234	0.	0.8		-102.0 ± 5.0
PN G347.7+02.0	17 04 34	-37 53 13	Vd 1-8	347+01.1	17011-3749	VANDERVORT 1964	ESO 332-18, Sa 2- 167	0.
PN G348.0+06.3	16 48 48	-35 00 57	MGP 1			MANCHADO et al 1989	RPZM 2- 1, Wray 15-1537		3.8					B: 18.2
PN G348.4-04.1	17 32 48	-40 58 24	H 1-21	348-04.1	17292-4056	HARO 1952	ESO 333-13, Sa 2-213, VV' 211, Wray 16- 284	0.
PN G348.8-09.0	17 56 33	-43 03 17	He 2-306	348-09.1	17529-4302	HENIZE 1964	ESO 279-12, Sa 2-267, StWr 2-29, Wray 16- 330	3.						B: 16.4, V: 16.8
PN G349.2-03.5	17 32 20	-39 51 20	H 2-14	349-03.1		HARO 1952	ESO 333-11, Sa 3- 62, RPZM 2-22, VV' 210	20. :	15.
PN G349.3-01.1	17 22 16	-38 28 58	NGC 6337	349-01.1	17188-3826	HERSCHEL 1834	ESO 333-05, H 1-10, He 2- 215, Sa 2- 191, Sh 1- 6, VV' 181, Wray 16- 267	51.			-71.0 ± 4.0	7.8 (O-III)	AG82 236	B: 15.5, V: 14.90
PN G349.3-04.2	17 35 40	-40 12 00	Lo 16		17322-4009	LONGMORE 1977		83.					AG82 248	B: 17.3, V: 16.8
PN G349.5+01.0	17 13 44	-37 06 06	NGC 6302	349+01.1	17103-3702	FLEMING 1896	ARO 502, ESO 392-05, Gum 60, He 2- 204, RCW 124, Sa 2- 180, Sh 1- 3, Sh 2- 6, VV 94, VV' 168, Wray 16- 259	44.5	10.		-39.0 ± 2.1	8.0 (O-III)	AG82 233, CD -36 11341, CPC 18 8579, GCRV 9926, HD 155520	B: >21.1
PN G349.8+04.4	17 01 06	-34 49 39	M 2- 4	349+04.1	16578-3445	MINKOWSKI 1947	ESO 391-07, He 2- 188, Sa 2-163, VV 84, VV' 150, Wray 16- 2456	< 5.	2.		-184.0 ± 11.0			B: 17.6, V: 17.0
PN G350.1-03.9	17 36 30	-39 22 02	H 1-26	350-03.1	17330-3920	HARO 1952	ESO 334-01, He 2- 253, Sa 2-220, VV' 220, Wray 16- 291	18.			-37.0 ± 5.0
PN G350.5-05.0	17 42 54	-39 36 28	H 1-28	350-05.1	17394-3935	HARO 1952	ESO 334-05, He 2- 268, Sa 2-231, VV4 233, Wray 15-1760	7.8			-45.0 ± 5.0
PN G350.8-02.4	17 32 20	-37 57 38	H 1-22	350-02.1	17289-3755	HARO 1952	ESO 333-12, He 2- 241, Sa 2-212, VV' 212, Wray 16- 283	0.			-213.0 ± 5.0
PN G350.9+04.4	17 04 37	-33 59 12	H 2- 1	350+04.1	17013-3355	HARO 1952	MWC 247, ESO 392-02, He 2- 194, SaSt 2- 14, VV' 155, Wray 16- 247	5.6	2.2	4.6	-20.0 ± 5.5	13.0 (O-III)	AG82 223	B: 13.66, V: 13.26	O(H)
PN G351.1+04.8	17 03 46	-33 29 52	M 1-19	351+04.1	17005-3325	MINKOWSKI 1946	ESO 392-01, He 2- 191, Sa 2-165, VV' 153, Wray 15-1601	8. :	2.6		-40.0 ± 11.0			B: 16.9
PN G351.2+05.2	17 02 19	-33 10 04	M 2- 5	351+05.1	16590-3305	MINKOWSKI 1947	ESO 391-08, He 2- 190, SaSt 2-13, VV 86, VV' 152, Wray 16- 246	5.	5.		-98.0 ± 11.0			B: 16.4, V: 16.2
PN G351.3+07.6	16 53 37	-31 40 35	H 1- 4	351+07.1		HARO 1952	ESO 453-09, Sa 2-158, VV' 147, Wray 16- 240	0.						B: 16.3, V: 16.3
PN G351.6-06.2	17 50 44	-39 17 24	H 1-37	351-06.1	17472-3916	HARO 1952	ESO 334-09, He 2- 291, Sa 2-251, VV' 262, Wray 16- 314	8.6			-16.0 ± 5.0
PN G351.9+09.0	16 50 17	-30 19 55	PC 13	351+09.1	16471-3014	PEIMBERT et al 1961	ESO 453-06, Sa 2-155, StWr 4- 3, Wray 16- 236	7. :						B: 16.7, V: 16.0
PN G351.9-01.9	17 33 00	-36 43 53	Wray 16-286		17296-3641	WRAY 1966	ESO 393-06, Sa 2-215	0.
PN G352.0-04.6	17 45 07	-38 08 49	H 1-30	352-04.1	17416-3807	HARO 1952	ESO 334-06, He 2- 272, VV' 237, Sa 2-23, Wray 16- 301	5.4			-8.0 ± 5.0
PN G352.1+05.1	17 05 31	-32 32 09	M 2- 8	352+05.1	17022-3228	MINKOWSKI 1947	ESO 453-18, He 2- 197, Sa 2-170, VV 91, VV' 158, Wray 16- 248	4.2	3.7		+26.8 ± 11.8
PN G352.6+00.1	17 26 24	-35 01 46	H 1-12	352+00.1	17230-3459	HARO 1952	ESO 392-12, He 2- 222, Sa 3- 51, VV' 190, Wray 16-273	6.8	11.
PN G352.6+03.0	17 14 43	-33 24 48	H 1- 8	352+03.2		HARO 1952	ARO 549, ESO 392-06, Sa 2-182, VV' 170	3.4
PN G352.8-00.2	17 28 27	-35 07 43	H 1-13	352-00.1	17251-3505	HARO 1952	ESO 393-01, He 2- 227, Sa 3-55, VV' 195, Wray 15-1712	9.6	14.
PN G352.9+11.4	16 44 49	-28 04 05	K 2-16		16416-2758	KOHOUTEK 1977	ESO 453-02, Wray 17- 76, Anon 16h38	23.					AG82 215	B: 13.18, V: 12.75	WC 11
PN G352.9-07.5	18 00 12	-38 49 52	Fg 3	352-07.1	17567-3849	FLEMING 1911	ARO 520, ESO 334- 10, He 2- 320, Sa 2-277, StWr 2-26, VV 133, VV' 308, Wray 16- 346	2.			+4.6 ± 2.0			B: 14.3, V: 14.3
PN G353.2-05.2	17 50 45	-37 23 54	H 1-38	353-05.1		HARO 1952	ESO 393-35, Sa 3- 81, VV' 264, Wray 16- 315	7.
PN G353.3+06.3	17 04 18	-30 53 29	M 2- 6	353+06.2	17012-3049	MINKOWSKI 1947	ESO 453-16, He 2- 192, Sa 2-166, VV 88, VV' 154	8. :	1.6		-88.7 ± 14.4			B: 16.67, V: 16.40
PN G353.5-04.9	17 49 48	-37 01 27	H 1-36	353-04.1	17463-3700	HARO 1952	ESO 393-31, He 2- 289, Sa 2-249, VV' 259	0.			-120.9 ± 3.1			V: 16.8
PN G353.7+06.3	17 05 14	-30 32 28	M 2- 7	353+06.1	17020-3028	MINKOWSKI 1947	ESO 453-17, He 2- 196, Sa 2-169, VV 90, VV' 157, Wray 15-1509	7.8			-56.0 ± 11.0			B: 14.72, V: 13.96
PN G354.2+04.3	17 14 07	-31 19 42	M 2-10	354+04.1	17108-3116	MINKOWSKI 1947	ESO 454-01, He 2- 205, VV 95, VV' 169, Wray 15-1647	4.	4.		-75.0 ± 11.0
PN G354.5+03.3	17 18 52	-31 39 06	Th 3- 4	354+03.1	17156-3135	THE 1964	ESO 454-07, Sa 3- 44	0.
PN G354.9+03.5	17 19 20	-31 12 34	Th 3- 6	355+03.3	17161-3109	THE 1964	ESO 454-09, Sa 3- 45	0.
PN G355.1+02.3	17 24 26	-31 43 18	Th 3-11	355+02.3	17212-3140	THE 1964	ESO 454-18, Sa 3- 47	0.
PN G355.1-02.9	17 45 32	-34 33 56	H 1-31	355-02.4	17422-3432	HARO 1952	ESO 393-21, He 2- 276, Sa 2-238, VV' 240, Wray 16- 305	< 5.	0.7		+86.0 ± 11.0
PN G355.2-02.5	17 44 14	-34 17 28	H 1-29	355-02.2	17409-3416	HARO 1952	ESO 193-16, He 2- 270, Sa 2-233, VV' 235, Wray 16- 299	0.			-18.0 ± 5.0				WC
PN G355.4-02.4	17 44 20	-34 06 41	M 3-14	355-02.1	17410-3405	MINKOWSKI 1948	ARO 552, ESO 393-19, He 2- 271, Sa 2-234, VV' 236, Wray 16- 300	7.2	2.8		-76.0 ± 11.0
PN G355.4-04.0	17 51 12	-34 55 26	Hf 2-1	355-04.1	17478-3454	HOFFLEIT 1953	ESO 393-37, Pe 1-10, Sa 2-253, VV' 266, Wray 16-316	9.4	12.
PN G355.6-02.7	17 46 06	-34 03 46	H 1-32	355-02.3	17427-3402	HARO 1952	ESO 393-23, He 2- 278, Sa 2-241, VV' 245, Wray 16- 307	< 5.	1.		-188.0 ± 5.0
PN G355.7-03.0	17 47 50	-34 08 00	H 1-33	355-03.1		HARO 1952	ESO 393-26, He 2- 283, VV' 248	0.	2.7		-117.0 ± 5.0
PN G355.7-03.4	17 48 58	-34 21 55	H 2-23	355-03.2		HARO 1952	ESO 393-27, He 3-1489, Sa 2-246, VV' 255	0.						B: 18.4, V: 17.7
PN G355.7-03.5	17 49 14	-34 22 53	H 1-35	355-03.3	17459-3421	HARO 1952	ESO 393-29, He 2- 288, My 103, Sa 2-247, VV' 257, Wray 16- 311	2.	1.1		+160.0 ± 11.0			B: 15.7, V: 15.4
PN G355.9+02.7	17 24 40	-30 51 53	Th 3-10	355+02.2	17214-3049	THE 1964	ESO 454-21, Sa 3- 48	0.	2.
PN G355.9+03.6	17 21 32	-30 20 48	H 1- 9	355+03.2	17183-3017	HARO 1952	AS 226, ESO 454-14, He 2- 213, VV' 176, Wray 15-1689, MHa 76- 33, EM* AS 226, Sa 2- 190	7. :	0.7		-148.0 ± 11.2	> 40.0 (O-III)		B: 16.6, V: 15.8
PN G355.9-04.2	17 52 59	-34 38 23	M 1-30	355-04.2	17496-3437	MINKOWSKI 1946	ESO 394-05, He 2- 295, Sa 2-259, VV 120, VV' 271, Wray 16- 322	< 5.	3.5		-98.0 ± 11.0			B: 16.6, V: 16.4	WC ?
PN G356.1+02.7	17 25 19	-30 40 44	Th 3-13	356+02.1	17221-3038	THE 1964	ESO 454-24	0.	< 2.
PN G356.1-03.3	17 49 51	-34 00 16	H 2-26	356-03.1		HARO 1952	ESO 393-32, Sa 3- 79, VV' 261, Wray 17- 99	4.5
PN G356.2-04.4	17 54 33	-34 22 21	Cn 2-1	356-04.1	17512-3421	CANNON 1922	ESO 394-10, He 2- 303, Sa 2-263, VV 126, VV' 281, Wra y 16- 327	2.4	1.7		-271.0 ± 25.0
PN G356.5+01.5	17 30 59	-31 01 08	Th 3-55	356+01.2	17277-3058	THE 1964	ESO 455-10, Sa 3- 58	0.	< 9.
PN G356.5-02.3	17 46 45	-33 08 35	M 1-27	356-02.2	17434-3307	MINKOWSKI 1946	ESO 393-24, He 2- 280, VV 113, VV' 246, Wray 16- 308	5.3	8.		-16.5	8.5 (O-III)	AG82 262, SS73 102	B: 15.58, V: 14.54
PN G356.5-03.6	17 51 50	-33 47 37	H 2-27	356-03.2	17485-3346	HARO 1952	ESO 394-02, Sa 3- 83, VV' 269	0.
PN G356.5-03.9	17 53 21	-33 56 00	H 1-39	356-03.3	17500-3355	HARO 1952	ESO 394-07, He 2- 300, VV' 277, Wray 16- 323	< 5.	1.7		-50.0 ± 11.0			B: 16.8, V: 16.3
PN G356.7-04.8	17 57 19	-34 09 49	H 1-41	356-04.2	17539-3409	HARO 1952	AS 256, ESO 394-13, He 2- 308, MHa 304- 10, Sa 2-269, VV' 293, Wray 16- 333	9.6			+76.0 ± 5.0			B: 16.3, V: 16.2
PN G356.8-05.4	18 00 19	-34 27 42	H 2-35	356-05.1		HARO 1952	ESO 394-17, Sa 3-109, VV' 311	10.8			-195.0 ± 5.0
PN G357.1+01.9	17 30 51	-30 17 14	Th 3-24	357+02.7		THE 1964	ESO 455-09	0.
PN G357.1-04.7	17 58 15	-33 47 39	H 1-43	357-04.3	17549-3347	HARO 1952	ESO 394-15, He 2- 313, VV' 297, Wray 16-335	2.	3.		+76.0 ± 11.0			B: 15.91, V: 15.42
PN G357.2+01.4	17 33 17	-30 26 31	Al 2-H			ALLEN 1979		0.
PN G357.2+02.0	17 31 07	-30 10 37	H 2-13	357+02.6		HARO 1952	ESO 455-12, VV' 209, Sa 3- 59, Wray 17- 86	0.
PN G357.2-04.5	17 57 25	-33 35 43	H 1-42	357-04.1	17541-3335	HARO 1952	ESO 394-14, He 2- 310, Sa 2- 270, VV' 294, Wray 16- 334	5.8			-79.0 ± 5.0			B: 17.3
PN G357.4-03.2	17 52 34	-32 45 52	M 2-16	357-03.2	17492-3245	MINKOWSKI 1947	ESO 394-04, He 2- 297, Sa 2- 256, VV 121, VV' 273, Wray 16- 320	5.4	2.2		+106.0 ± 11.0
PN G357.4-03.5	17 53 38	-32 58 53	M 2-18	357-03.4	17503-3258	MINKOWSKI 1947	ESO 394-08, He 2- 301, Sa 2- 261, VV 124, VV' 278, Wray 16- 324	< 5.	1.5		-3.0 ± 11.0			B: 17.7, V: 17.3
PN G357.4-04.6	17 58 33	-33 28 37	M 2-22	357-04.2	17552-3328	MINKOWSKI 1947	ESO 394-16, He 2- 316, Sa 2-273, VV 132, VV' 302, Wray 16- 341	5.2	5.		-92.0 ± 11.0			B: 17.3, V: 16.5
PN G357.6+01.0	17 35 44	-30 21 29	TrBr 4			TERZAN et al 1978	TeJu 21	30.			-122. ± 60.
PN G357.6-03.3	17 53 17	-32 40 41	H 2-29	357-03.3	17499-3240	HARO 1952	ESO 394-06, Sa 3- 87, VV' 276	4.8					AG82 268	B: >21.
PN G357.9-03.8	17 56 14	-32 37 34	H 2-30	358-03.2	17529-3236	HARO 1952	ESO 394-11, VV' 287	11.2					AG82 273	B: >21.
PN G357.9-05.1	18 01 22	-33 17 44	M 1-34	357-05.1	17580-3317	MINKOWSKI 1946	ESO 394-18, He 2- 324, Sa 2-279, VV 135, VV' 313, Wray 16- 348	11.2			+2.0 ± 11.0
PN G358.2-01.1	17 46 03	-31 03 32	Bl D	358-01.1		BLANCO 1961	Al 2- L, ESO 455-34, Wray 17- 98	13.
PN G358.3-02.5	17 51 45	-31 36 00	Al 2-O		17484-3135	ALLEN 1979			2.4		-85.0
PN G358.5-02.5	17 52 10	-31 30 03	M 4- 7	358-02.1		MINKOWSKI 1948	ESO 455-54, Al 2-P	7.	5.7
PN G358.5-04.2	17 59 02	-32 21 44	H 1-46	358-04.1	17557-3221	HARO 1952	ESO 456-31, He 2- 318, Sa 2-274, VV' 306, Wray 16- 342	0.	1.2		-13.1 ± 10.1			B: 16.8, V: 16.2
PN G358.7-02.7	17 53 37	-31 25 33	Al 2-R			ALLEN 1979		0.
PN G358.9-00.7	17 45 58	-30 12 00	M 1-26	358-00.2	17427-3010	MINKOWSKI 1946	Bl C, AS 270, ESO 455-33, He 2- 277, RCW 135, SaSt 2-17, VV 112, VV' 242, Wray 16- 306	4.2		1.9	-5.0 ± 11.0	13.5 (O-III), 5.5 (N-II)	AG82 260, HD 316248, MWC 270	B: 13.44, V: 12.72	Of(H)
PN G358.9-03.7	17 58 11	-31 42 57	H 1-44	358-03.1	17549-3142	HARO 1952	ESO 456-23, He 2- 314, RCW 136, Sa 3-101, VV' 299, Wray 16- 336	3.6			+99.0 ± 5.0
PN G359.0-04.1	17 59 57	-31 54 34	M 3-48	359-04.1		MINKOWSKI 1948	ESO 456-34, Sa 3-108, VV' 310, Wray 16- 345	4.9			-11.0 ± 5.0		AG82 277	B: >21.
PN G359.1-01.7	17 50 18	-30 34 55	M 1-29	359-01.1	17471-3034	MINKOWSKI 1946	Bl F, ESO 455-47, He 2- 292, Sa 2-250, VV 119, VV' 263, Wray 16- 313	7.6	7.		-62.0 ± 11.0
PN G359.1-02.3	17 52 47	-30 49 45	M 3-16	359-02.2	17495-3048	MINKOWSKI 1948	VV' 272, Sa 2-258, ESO 456-02, Wray 16- 321, He 2- 296, Bl J=K	8.2	6.5		+81.0 ± 11.0			B: 18.0, V: 17.2
PN G359.1-02.9	17 55 06	-31 12 22	M 3-46	359-02.4	17518-3111	MINKOWSKI 1948	ESO 456-15, Sa 3- 93, VV' 283, Wray 17- 103	4.2						V: 17.9
PN G359.3-01.8	17 51 19	-30 23 54	M 3-44	359-01.2	17480-3023	MINKOWSKI 1948	Bl H, ESO 455-51, Sa 3- 82, VV' 267, Wray 16- 317	4.4	4.		-89.0 ± 11.0
PN G359.3-03.1	17 56 26	-31 04 23	M 3-17	359-03.1	17531-3103	MINKOWSKI 1948	ESO 456-21, He 2- 307, Sa 3- 97, VV' 289, Wray 16- 331	< 5.	2.9		-28.0 ± 11.0			B: 18.1, V: 17.1
PN G359.4-03.4	17 58 13	-31 08 08	H 2-33	359-03.2	17549-3107	HARO 1952	ESO 456-25, Sa 3-102, VV' 298, Wray 16- 338	6.2					AG82 275	B: >21.
PN G359.7-01.8	17 52 05	-30 05 18	M 3-45	359-01.3	17489-3004	MINKOWSKI 1948	Bl I, ESO 455-53, Sa 3- 84, VV' 270, Wray 17- 100	6.0	6.6		+32.0 ± 11.0
PN G359.7-02.6	17 55 36	-30 33 32	H 1-40	359-02.3	17523-3033	HARO 1952	Bl 3-8, ARO 29, ESO 456-17, Sa 2-266, VV' 286, Wray 16- 328	3.8	1.3		+108.0 ± 11.0

«A Catalog of Parameters for Globular Clusters in the Milky Way» William E. Harris, 1996 ^[148]
ID	Name	RA	Dec	R_Sun	R_GC	Fe/H	wt	E_B-V	V_HB	(m-M)V	V_t	M_V,t	U-B	B-V	V-R	V-I	spt	ellip	v_r	v_LSR	sig_v	c	r_c	r_h	μ_V	ρ₀	lg(tc)	lg(th)
NGC 6093	M 80	16 17 02.41	-22 58 33.9	10.0	3.8	-1.75	6	0.18	16.10	15.56	7.33	-8.23	0.21	0.84	0.56	1.11	F6	0.00	8.1 ± 1.5	16.7	12.4 ± 0.6	1.68	0.15	0.61	15.11	4.79	7.78	8.80
NGC 6121	M 4	16 23 35.22	-26 31 32.7	2.2	5.9	-1.16	11	0.35	13.45	12.82	5.63	-7.19	0.43	1.03	0.69	1.42	F8	0.00	70.7 ± 0.2	78.6	4.0 ± 0.2	1.65	1.16	4.33	17.95	3.64	7.90	8.93
NGC 6144		16 27 13.86	-26 01 24.6	8.9	2.7	-1.76	4	0.36	16.40	15.86	9.01	-6.85	0.35	0.96	0.60	1.10	F5/6	0.25	193.8 ± 0.6	201.9		1.55	0.94	1.63	20.05	2.31	8.78	9.14
NGC 6139		16 27 40.37	-38 50 55.5	10.1	3.6	-1.65	2	0.75	17.90	17.35	8.99	-8.36	0.73	1.40	0.91	1.86	F6/7	0.05	6.7 ± 6.0	11.5		1.86	0.15	0.85	17.20	4.67	7.66	9.05
Terzan 3		16 28 40.08	-35 21 12.5	8.2	2.5	-0.74	2	0.73	17.51	16.82	12.00	-4.82							-136.3 ± 0.7	-130.6		0.70	1.18	1.25	22.52	1.82	8.79	8.57
1636-283	ESO452-SC11	16 39 25.45	-28 23 55.3	8.3	2.1	-1.50	1	0.46	16.60	16.02	12.00	-4.02										1.00	0.50	0.50	20.75	2.50	8.07	7.87
NGC 6256		16 59 32.62	-37 07 17.0	10.3	3.0	-1.02	2	1.09	19.09	18.44	11.29	-7.15	1.03	1.69					-101.4 ± 1.9	-95.6	6.6 ± 2.6	2.50 c	0.02	0.86	17.89	5.59	5.82	8.86
Terzan 2	HP 3	17 27 33.10	-30 48 08.4	7.5	0.8	-0.69	3	1.87	20.87	20.17	14.29	-5.88							109.0 ± 15.0	116.9		2.50 c	0.03	1.52	22.16	4.86	5.46	8.82
Terzan 4	HP 4	17 30 39.00	-31 35 43.9	7.2	1.0	-1.41	4	2.00	21.07	20.48	16.00	-4.48							-50.0 ± 2.9	-42.3		0.90	0.90	1.85				8.70
Liller 1		17 33 24.50	-33 23 20.4	8.2	0.8	-0.33	4	3.07	24.84	24.09	16.77	-7.32							52.0 ± 15.0	59.2		2.30	0.06		24.00	5.28	6.62	0.00
NGC 6380	Ton 1	17 34 28.0	-39 04 09	10.9	3.3	-0.75	2	1.17	19.50	18.81	11.31	-7.50		2.01					-3.6 ± 2.5	2.1		1.55 c:	0.34	0.74	19.89	3.73	8.40	8.86
Terzan 1	HP 2	17 35 47.8	-30 28 11	6.7	1.3	-1.03	3	1.99	20.96	20.31	15.90	-4.41							114.0 ± 14.0	122.0		2.50 c	0.04	3.82	25.09	3.85	4.99	9.12
Ton 2	Pismis 26	17 36 10.5	-38 33 12	8.2	1.4	-0.70	1	1.24	19.10	18.41	12.24	-6.17							-184.4 ± 2.2	-178.6		1.30	0.54	1.30	22.16	2.85	8.23	8.82
NGC 6388		17 36 17.23	-44 44 07.8	9.9	3.1	-0.55	6	0.37	16.85	16.13	6.72	-9.41	0.66	1.17	0.71	1.47	G2	0.01	80.1 ± 0.8	84.2	18.9 ± 0.8	1.75	0.12	0.52	14.49	5.37	7.72	8.90
Djorg 1		17 47 28.3	-33 03 56	13.7	5.7	-1.51	1	1.58	21.15	20.58	13.60	-6.98							-362.4 ± 3.6	-355.0		1.50	0.50	1.59	23.10	2.68	8.71	0.00
NGC 6441		17 50 13.06	-37 03 05.2	11.6	3.9	-0.46	6	0.47	17.51	16.78	7.15	-9.63	0.81	1.27	0.79	1.62	G2	0.02	16.5 ± 1.0	22.9	18.0 ± 0.2	1.74	0.13	0.57	14.85	5.26	7.93	9.09
Terzan 6	HP 5	17 50 46.38	-31 16 31.4	6.8	1.3	-0.56	2	2.35	22.16	21.44	13.85	-7.59							126.0 ± 15.0	133.9		2.50 c	0.05	0.44	20.76	5.83	6.46	8.22
NGC 6453		17 50 51.70	-34 35 57.0	11.6	3.7	-1.50	4	0.64	17.88	17.30	10.08	-7.22	0.68	1.31	0.99	2.00	F8	0.09	-83.7 ± 8.3	-76.7		2.50 c	0.05	0.44	17.07	4.95	6.73	8.52
NGC 6496		17 59 03.68	-44 15 57.4	11.3	4.2	-0.46	3	0.15	16.47	15.74	8.54	-7.20	0.45	0.98			G4	0.16	-112.7 ± 5.7	-108.4		0.70	0.95	1.02	20.17	1.99	8.94	9.04

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61	Eye On The Sky: Scorpius by Deborah Byrd; Astronomy 6/93, p.48
107	Rabbit Tracks by E. C. Krupp; S&T 6/94, p.64
141	Strasbourg-ESO Catalogue of Galactic Planetary Nebulae; A. Acker, F. Ochsenbein, B. Stenholm, R. Tylenda, J. Marcout, C. Schohn; European Southern Observatory; ISBN 3-923524-41-2 (1992); Bibcode:1992secg.book.....A; cdsarc.u-strasbg.fr/viz-bin/cat/V/84
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150	IAU: The Constellations, 11. Oktober 2020; iau.org/public/themes/constellations
154	Yale Bright Star Catalog, 15. Oktober 2020; tdc-www.harvard.edu/catalogs/bsc5.html
265	PP3 - Celestial Chart Generation, Torsten Bronger; pp3.sourceforge.net (2021-02-11)
277	«Historische Deep-Sky Kataloge» von Dr. Wolfgang Steinicke; klima-luft.de/steinicke (2021-02-17)