Constellation Perseus (Hero)

Perseus
Perseus: IAU Constellation Map [150]

Properties

Perseus lies east of Andromeda and southeast of Cassiopeia. The band of the Milky Way runs through this constellation and is darkened there by a large cloud of dust. Despite its glorious legend, Perseus is a figuratively difficult to understand constellation. The most striking is the small, elongated group of stars around Algenib. To the south of this is the bright, short-period variable star Algol, which is therefore also called devil's eye and represents the severed Medusa head. The area of the constellation is 615 square degrees and the center culminates around midnight on November 7th. [9, 15]

Stars with Proper Names:

  • α Per: Mirphak, Mirfak, Marfak, Algenib
  • β Per: Algol, Gorgona, Gorgonea Prima, Demon Star, El Ghoul
  • η Per: Miram
  • ξ Per: Menkib, Menkhib, Menchib
  • ο Per: Atik, Ati, Al Atik
  • π Per: Gorgonea Secunda
  • ρ Per: Gorgonea Tertia
  • ω Per: Gorgonea Quarta
Data for constellation Perseus [150]
IAU NamePerseus
IAU GenitivePersei
IAU Abbr.Per
English NameHero
Season (47° N)August … March
Right Ascension01h 29m 38s … 04h 51m 22s
Declination+30° 55' 19" … +59° 06' 17"
Area615 deg2
Neighbours (N↻)Cas, And, Tri, Ari, Tau, Aur, Cam

Deep-Sky Object Descriptions

Mythology and History

Akrisios was the king of Argos and had a lovely daughter named Danae. The Oracle of Delphi prophesied that his grandson would one day kill him. For fear of this oracle, Akrisios had his daughter Danae locked in a tower so that she could not receive a husband. Of course, Akrisios could not have known that Zeus himself wanted to approach the lovely Danae. Zeus did this too and took the form of a golden rain that penetrated through the walls, joints, cracks and windows. Danae gave birth to a son, who was called "The one who emerged from flowing gold" or "The one who was born in gold" - Perseus. Akrisios didn’t keep this hidden for long, of course, and had his daughter and grandchild nailed into a box, which was then thrown into the sea.

Constellation Perseus
Constellation Perseus: Illustration from «Uranometria» by Johann Bayer, copper engraving by Alexander Mair, 1603 [28]

Danae and Perseus drifted for a long time until they finally stranded on the coast of the stony island of Seriphos and were freed from their prison. On this island, Polydektes ruled, who soon campaigned for the beautiful Danae for years, but in vain. Either to force Danae into marriage after all, or to get Perseus out of the way, he sent Danae's son, who had meanwhile grown into a youth, to do a deadly task. He should get the head of Medusa.

Medusa was one of the Gorgons, one of the three daughters of Phorkys, who were equipped with snake hair and could cast a petrifying look. Two of these daughters were immortal, while Medusa was mortal. This father also had three other daughters, the Graien, "the ancient ones", who all together had only one eye and one tooth, which they had to borrow alternately if needed.

With the help of Hermes' winged shoes, the hat of Hades, which spread the impenetrable night, and the sickle sword of the limping fire and blacksmith god Hephaestus, Perseus succeeded in overcoming the Graien. He took away their only eye when the second of the three sisters wanted to see something. The way was cleared and he penetrated the Gorgons with the Hades cap pulled over his head. Perseus was careful not to look directly at Medusa, but only to look at her reflection in his polished shield - otherwise he would have immediately turned to stone. In this way he managed to behead Medusa, who was pregnant by Poseidon. The winged horse Pegasus then rose from the dead body. Even the grown-up warrior Chrysaor with a golden sword in hand emerged from her dead body. Perseus put the Gorgon head, which was still dripping with blood, into the magic sack and escaped with the help of the Hades cap, which spread deep darkness all around.

Constellation Monoceros
Constellation Monoceros: Illustration from «Prodromus Astronomiae» by Johannes Hevelius, 1690. Mirrored view from «outside of the celestial sphere» [19]

Perseus passed the coast of Ethiopia on his way back. There was the beautiful Andromeda - the daughter of the queen Kassiopeia and the king Kepheus - helpless and almost naked, only wearing a few pieces of jewelry, chained to a rock. A dreadful sea monster approached her with the intention of devouring her. Perseus immediately fell in love with the beautiful princess. He seized the opportunity and asked Andromedas father, King Cepheus of Ethiopia, that Hand of his daughter and a kingdom of her own to save her. He agreed, fearing for his daughter's life. Then Perseus put on his winged shoes and hurried through the air in the direction of sea monsters. Everything he did was designed to get this girl's attention to himself. The liberation took place only armed with the sword. [20] More common, however, is the variant in which he took Medusa's head out of the sack and petrified the sea monster into a rock in the sea. [66]

Perseus hurried back to his home island Seriphos and appeared in front of Polydectes. He shouted: "Here is your present!" and held up Medusa's head. Instantly the king and his followers froze to stone. Perseus returned to his lover Andromeda and married her. Both lived long and happily and had many children. One of her great-grandchildren was Hercules. When Perseus died, he was granted a place under the stars in the sky: his sword stretched up and the diabolical head of Medusa held in the other hand, so that she might look upon humanity for all time. [66]

Some names like Perseus, Perseus et Caput Medusae, Victor Gorgonei monstri, Gorgonifer are reminiscent of the story and Bearer of Medusa Head. This star formation was also transformed into biblically oriented images such as David with the head of Goliath and Apostle Paul with sword and book. [20]

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 470BD+53 3631011022493I 01 40 13.1+53 52 066.39 K5III
HR 496φBD+49 444105162255457I Phi Per01 43 39.6+50 41 194.07 B2Vep G:In neutral hydrogen region; Cas-Tau OB1.,P:Intrinsic polarization, probably due to circumstellar matter.,S:FeII, H in emission. Also classified B0nne, B1III-Vpe.,SB:126.696d. Primary, 16.8k/s, V0 -8.4k/s, msin3i 21.1, asini 29.2; secondary K 105.3k/s, sin3i 3.4,,SB:asini 184. Unresolved by speckle interferometry. Both components appear to be shell stars, B2Ve and B3Ve. Speculation,SB:that secondary is the helium core of a once more massive star whose mass was transferred to the primary.,VAR:Gamma Cas 4.03 - 4.11V, 19.5d. Amp. varies in per. 127d. Possible mass loss. Expanding circumstellar shell.
HR 526BD+47 50811031375361438 01 49 15.7+47 53 495.82 A3V 0.71.9D:Component C 8.4v at 21", D 10.2v at 137".,SB:ADS 1438B.
HR 529BD+51 4161115122678 01 50 57.1+51 56 005.90 F5IV
HR 5331BD+54 39611241226902122 V436 Per01 51 59.3+55 08 515.52 B1.5V G:In neutral hydrogen region; Cas-Tau OB1.,SB:15.6d, K 10k/s, V0 -9k/s.,VAR:E? 5.46 - 5.68y.
HR 5362BD+50 37911291226961052 01 52 09.4+50 47 345.79 B9IIIpHgMn SB:5.6270d, K 26.5k/s, V0 +11.4k/s, asini 2.05.
HR 538BD+50 3811133522705 01 52 50.8+51 28 296.26 A3V
HR 540BD+54 4081140822716 01 53 48.5+55 35 536.45 A5m
HR 5683BD+48 5761194937665 01 58 33.6+49 12 155.69 K0IV
HR 5904BD+53 43912303228591054 02 02 18.1+54 29 155.04 B8III
HR 618BD+57 4941295322959 V472 Per02 08 40.5+58 25 255.67 A1Ia tG:NGC 869; Per OB1.,S:Shell star.,VAR:Amp. 0.065V. Sp. var., H alpha profile var.
HR 621BD+53 46013137229932146 02 10 07.8+53 50 356.31 G8III
HR 6275BD+56 43813267230111685 Var?02 11 29.0+57 38 456.36 B5Ia 6.960.0D:B, mag. diff 6.9v at 5.6".,G:Per OB1; h Per.
HR 641BD+57 5191347623044 02 13 41.5+58 33 406.44 A3Iab G:Per OB1; h Per.
HR 654BD+56 4711385423115W Var?02 16 51.7+57 03 196.48 B1Iab e0.9103.0G:NGC 869 = h Per; Per OB1.
HR 6618BD+57 53513982231432157 02 17 59.9+57 53 595.75 K3III
HR 6627BD+56 48613994231491753 02 18 04.5+57 31 005.98 G7III 2.6121.9C:Heavily reddened.,G:May not be member of Per OB2.,N:Sometimes misidentified as Chi Per.
HR 6859BD+55 598144892325621591802 V474 Per02 22 21.4+55 50 445.17 A2Ia v7.811.6D:Fixed.,G:Per OB1.,RV:Var. in period over 200d.,S:Shell star.,VAR:Amp. 0.05V. Sp. and H alpha profile var.
HR 690BD+54 53514662232831820 V440 Per02 23 51.8+55 21 526.28 F7Ib 8.110.0VAR:CDelta, amp. 0.123V, 7.572d.
HR 69610BD+55 6121481823304 Var02 25 16.0+56 36 366.25 B2Ia eG:Per OB1; in cluster Chi Per; NGC 884.,VAR:Amp. at 0.58 micrometers about 0.15m.
HR 716BD+54 55715253233691878 02 29 25.0+55 32 116.51 A2pShell v1.32.8D:Companion A3IV.,VAR:ADS 1878A, spectrum variable, shell star.
HR 78511BD+54 59816727235552188 02 43 02.8+55 06 215.77 B7IIIpHg SB:Double lines suspected.
HR 787BD+52 61616735235562059 02 42 59.7+53 31 345.84 K0II-III 9.012.4D:Optical.
HR 78812BD+39 61016739557932187S 896 02 42 14.9+40 11 384.91 F9V 0.30.1D:0.906y, a = 0.057".,DYN:0.046".,SB:331.0d, K 21.4k/s, V0 -21.5k/s, msin3i 0.744, asini 72.3. Speckle interferometer measurements combined with,SB:spectroscopic yield masses 1.28 and 1.05 solar. Speckle interferometric sep. 0.047", 1981.68.
HR 792BD+47 68316780382742064 02 43 01.9+48 15 566.48 R G5II 5.072.8D:AB fixed.,G:UMa stream.
HR 799θ13BD+48 746168953828893I2081 902 02 44 12.0+49 13 424.12 F8V 5.619.6D:AB 4.13 F7V, 9.87 M1V, 2720y, a = 22.289". C probably optical.,DYN:0.095".
HR 80014BD+43 56616901382891077 02 44 05.2+44 17 495.43 G0Ib-IICa1CH-1
HR 819BD+35 5531722855868 02 46 58.3+35 59 016.25 G8III G:Probable Hyades group.
HR 820BD+34 51317240558722117 02 47 03.5+35 33 186.30 R A9V 2.11.5D:AB binary.
HR 825BD+56 7181737823637S V480 Per02 49 30.8+57 05 036.25 A5Ia G:Per OB1; vicinity of Perseus double cluster.,VAR:Amp. 0.038V.
HR 831BD+36 5661748455910 02 49 27.1+37 19 346.45 F6III-IV
HR 834η15BD+55 714175062365599I2157 02 50 41.8+55 53 443.76 K3-Ib-IIa e4.728.3C:Large infrared excess.,D:Component B, B9V, CPM, vsini 149k/s.,G:Red star Pleiades group.,N:Miram in Becvar; Allen says unnamed.,S:Ultraviolet FeII emission. Also classified K3Ib.
HR 84016BD+37 64617584559282194W 956 02 50 35.1+38 19 074.23 F2III 4.7249.3VAR:Delta Sct?
HR 842BD+46 64817656383972197 02 51 41.7+46 50 315.88 G8III
HR 84317BD+34 52717709559462198IA 963 02 51 30.8+35 03 354.53 K5+III S:Also classified K7III.
HR 846BD+52 64017743236742185 971 02 52 52.0+52 59 526.36 B8III 0.21.6D:AB, 7.2, 9.2v sep. 0.2" possibly optical; AC binary.,DYN:0.006".
HR 849BD+47 72317818384182192 02 53 21.2+48 34 106.26 G5I 5.76.7
HR 854τ18BD+52 6411787823685103I2202 Tau Per02 54 15.5+52 45 453.95 G4III+A4V 8.651.7D:A* 4.06 G4III+A4V, 4.150y, a = 0.050". Speckle interferometric sep. 0.080" 1981.67. Circumstellar material surrounding,D:the pair? Visual companions 10.7v at 51" possibly physical; 11.8v at 4" possibly optical.,SB:ADS 2202A, 1515.6d, K 19.0k/s, V0 +2.2k/s, asini 271. vsini of secondary 50k/s.,VAR:EA, 3.94 - 4.07V.
HR 85520BD+37 65517904559752200 977 02 53 42.6+38 20 155.33 F4IV 0.60.2D:AB 5.9 F4V, 6.5 F6V, 31.37y, a = 0.258". Nearly equal components, 3.7, 4.3 solar. Component C, 9.7v at 14", CPM?,DYN:0.013".,SB:ADS 2200A, 1269d, K 4.8k/s, V0 +2.4k/s, asini 73.0. Orbit questioned by Morbey and Griffin (1987, ApJ, 317,,SB:343). Resolved by speckle interferometry 1983.93, sep. 0.20"; 1983.94, sep. 0.18".,VAR:Delta Sct?
HR 864BD+50 6651815323721 02 56 50.6+51 15 396.22 K5III
HR 865BD+46 6581815538455W 02 56 33.4+47 09 506.02 gK3 5.524.9D:Component B, 15v, possibly spurious.
HR 87321BD+31 50918296560312205 LT Per02 57 17.3+31 56 035.11 B9pSi vG:Member moving cluster in Perseus.,S:Underabundance of magnesium and oxygen.,SB:2.88d.,VAR:Alpha CV 5.03 - 5.14V, 2.88422d, same for RV and line-intensities. Also var. magnetic field and H-lines. Rotating,VAR:spotted star.
HR 876BD+38 5991833956036I 02 58 02.3+38 36 546.04 gK3
HR 879π22BD+39 68118411560472207 02 58 45.7+39 39 464.70 A2Vn N:Gorgonea Secunda.
HR 88224BD+34 55018449560521082I 02 59 03.7+35 10 594.93 K2III
HR 885BD+46 6691847438493 02 59 49.9+47 13 155.47 G5:III* S:G5:III: CN-4 CH-1 Ca 1 H delta-1. Also classified G8III CH weak. Noted as having composite spectrum, but unresolved,S:by speckle interferometry 1981.69.
HR 886BD+40 6391848238492I 1004 02 59 39.9+41 01 595.89 K2
HR 890BD+51 66518537237632270 A03 00 52.2+52 21 065.28 B7V 1.411.9D:CPM with HR 891.,G:Per OB3.
HR 891BD+51 66518538237652270 B03 00 53.4+52 21 086.74 B9V 1.411.9D:CPM with HR 890.,G:Per OB1?
HR 894BD+37 6751855256067 03 00 11.8+38 07 546.11 B8Vne S:Shell star. Near IR spectroscopy indicates presence of cool companion.
HR 915γ23BD+52 6541892523789108I2324 03 04 47.8+53 30 232.93 G8III+A2V 8.657.0D:SKYLAB observations indicate cool star with hot companion. Components Aa, 14.65y, a = 0.159". Physical nature of B,,D:11m at 57", uncertain.,M:Close to error box of X-ray source 3U0305+53.,SB:5350d, K 12.7 or 21.9k/s, V0 +2.5k/s, msin3i 4.87, asini 648. vsini of secondary 50k/s. Resolved by speckle,SB:interferometry 1981.67, sep. 0.284", 1983.93, sep. 0.27".
HR 918BD+56 76718970237912217I 03 05 32.4+56 42 214.76 G9.5III
HR 920BD+55 7381899123793 03 05 39.9+56 04 076.11 G9III
HR 921ρ25BD+38 6301905856138109I Rho Per03 05 10.6+38 50 253.39 M4II G:Zeta Her group.,N:Gorgonea Tertia.,VAR:SRb 3.30 - 4.0V, about 50d with possibly slow var. in mean brightness in 1100d period.
HR 923BD+40 6641906638559 03 05 20.8+40 34 576.05 K0III
HR 930BD+51 6811926823825 03 08 03.9+52 12 486.31 B5V
HR 933BD+46 6921927938587 03 07 47.4+47 18 306.41 A3Vnn
HR 936β26BD+40 6731935638592111I2362 Bet Per03 08 10.1+40 57 202.12 B8V 8.381.9C:Color excess E(B-V) = +0.03.,D:A* var. B8V, 1.858y, a = 0.011" or 1.862y, a = 0.104". Apparent apsidal period 28.4y or 32y. Resolved by speckle,D:interferometry: sep. 0.086", 2-3v fainter than primary. This may be Algol C. Four visual companions all optical:,D:B, 12.7v at 59"; C, 12.5 at 67"; D, 10.5 at 82"; BC sep. 15"; E, 12.5v at 11" from D.,M:One of the few known galactic radio sources in which the dominant star is normal. 21cm radio source.,N:ALGOL; Gorgona; Gorgonea Prima; Demon Star; El Ghoul.,S:B8V+G.,SB:Algol ABxC: 1.8613y, K 12.0k/s, V0 +3.7k/s, msin3i 3.91, asini 109. Spectra B8V, G5IV, Am. Mass Algol AB, 5.3,SB:Suns; C, 1.8 Suns. Circumstellar gas fills Roche lobe of hot component. ADS 19356A: 2.8673d, K 44.0k/s, V0 var.,,SB:asini 1.73. Resolved by speckle interferometry 1982.17, sep. 0.052", 1983.94, sep. 0.08".,VAR:ADS 2362A is the prototype Algol star, first discovered as variable by Montanari in 1669. The first period determined by,VAR:Goodricke in 1783, who also interpreted the variations as due to eclipses. The prototype star proves to be a more,VAR:a complicated system than most of the Algol-type stars, i.e., compact triple system with separation of the components,VAR:well under 0.1". The components usually designated Algol A, B, C, sometimes A, a, P. Two formerly additionally desig-,VAR:nated components D and E, inferred on the basis of an apparent 32 year apsidal motion, are now considered spurious.,VAR:The various Algol components must not be confused with the visual components ADS 2362 B-E, optical companions at much,VAR:greater distances from A. ADS 2362A, EA 2.12 - 3.40V, 2.86732442d, abrupt period changes. Orbital and rotation periods,VAR:synchronized. Rotational velocity 65k/s. Radio flares extending to about 1 A.U., not associated with X-ray activity.,VAR:Radio flare activity appears correlated with period discontinuities, attributed to "starquakes." Mass flow from K to B8,VAR:component at rate of 1.8x10E-08 solar masses/year. Possible circumstellar material associated with radio or H alpha,VAR:emission.
HR 937ιBD+49 8571937338597112IW 03 09 04.0+49 36 484.05 G0V 8.2146.2G:Mel 20 #44, but not cluster member; Per OB3.
HR 941κ27BD+44 6311947638609I2368 1055 03 09 29.8+44 51 263.80 K0III 8.427.7D:Companion optical.,G:Hyades group.
HR 947ω28BD+39 7241965656224IW 03 11 17.4+39 36 424.63 K1III 6.1177.4N:Gorgonea Quarta.
HR 949BD+47 77919735386382225IW 03 12 26.4+47 43 336.33 K5III 3.9202.1G:Mel 20 #138; Per OB3.
HR 950BD+41 6311973638635 03 12 09.6+42 22 346.15 B4V G:Member of the local association (Pleiades group).
HR 956BD+47 7821984538652 03 13 24.0+48 10 375.90 G9III G:Mel 20 #175; Per OB3. Nonmember of Alpha Per cluster on basis of RV.,M:Space motion same as for Hyades cluster.
HR 964BD+56 79820041239032424 03 15 48.0+57 08 275.79 A0Ia 8.210.8G:In reflection nebula; member assoc. Cam R1 at about 870 pc. Cam OB1.
HR 966BD+41 6382006338674 03 14 56.7+42 30 146.07 R K2III S:Strong CN.
HR 969BD+50 7292012323914I 03 16 12.2+50 56 165.03 G6Ib-IIa G:Mel 20 #308; Per OB3.,SB:5.543491d.
HR 973BD+44 6482016238685I 03 16 04.7+45 20 456.16 M2III
HR 975BD+32 59120193562932431 03 15 47.0+32 51 236.31 F4V vw 6.544.1
HR 976BD+34 61020210562962433 V423 Per03 16 01.9+34 41 196.25 A1m 7.229.3SB:ADS 2433A, 5.5435d, K 62.7k/s, V0 +24.2k/s, asini 4.78.,VAR:Ell 6.16 - 6.28V, 5.543491d.
HR 978BD+31 5762027756308 03 16 35.1+32 11 016.06 G8IV
HR 979BD+39 74320283387002443 03 17 11.4+40 29 006.45 B9VpSi 0.93.8D:Component B, 8.0 A7m. CPM.
HR 98230BD+43 6742031538704 03 17 47.4+44 01 305.47 B8V G:Per OB3; nonmember of Alpha Per cluster on basis of RV.
HR 986BD+38 69020346563222230 03 17 45.8+39 17 005.96 A2IV
HR 98729BD+49 8992036523944 03 18 37.8+50 13 205.15 B3V G:Per OB3.,SB:1.996933d.
HR 98931BD+49 9022041838714 03 19 07.6+50 05 425.03 B5V G:Per OB3.
HR 991BD+33 61920468563402232I 03 18 43.8+34 13 224.82 K2IICN1 S:Also classified K2III CN2 Ba 0.3.
HR 1001BD+48 8932067538753W 03 21 52.6+49 04 155.93 F6V 3.5205.8G:Hyades moving group; Per OB3; Mel 20 #497.
HR 100232BD+42 75020677387502236 1107 03 21 26.5+43 19 464.95 A3V
HR 1011BD+48 8992080938768 03 23 13.2+49 12 485.29 B5V G:Mel 20 #557; Per OB3; nebulosity.,SB:Possibly long period.
HR 1017α33BD+49 9172090238787120IW 1125 03 24 19.4+49 51 401.79 F5Ib 10.0167.0G:Mel 20 #605; Per OB3; nebulosity.,N:MIRPHAK; Mirfak; Marfak; Algenib.
HR 1019BD+33 63620995564192514 03 24 29.7+33 32 095.61 R A0V 3.54.3D:AB CPM.
HR 1020BD+53 6572100424024 03 25 48.4+53 55 186.51 A9III-IV
HR 1026BD+40 7362103838809 03 25 09.4+41 15 266.51 A0V
HR 1029BD+48 9132107138817 03 25 57.4+49 07 156.09 B7V G:Mel 20 #675; Per OB3.
HR 1034BD+48 9202127838849 03 28 03.1+49 03 464.98 B5V C:Color excess E(B-V) = +0.10.,G:Mel 20 #774; Per OB3.,S:Lyman alpha observed from COPERNICUS.,SB:21.659d, K 25.0, V0 -0.5, asini 7.34.
HR 1037BD+49 9442136238862 03 28 52.4+49 50 545.58 B6Vn G:Mel 20 #810; Per OB3.
HR 1041BD+33 6562140256475 03 28 20.8+33 48 275.61 R A2V
HR 104434BD+49 94521428388722558 03 29 22.1+49 30 324.67 B3V 2.10.8D:550y.,G:Mel 20 #835; Per OB3.
HR 1047BD+46 76021455388742560 03 29 26.2+46 56 166.24 B7V 5.127.9G:Mel 20 #861; Per OB3. Nonmember of Alpha Per cluster on basis of RV.
HR 1051BD+47 8442155138893 03 30 37.0+48 06 135.82 B8V G:Mel 20 #904; Per OB3.,S:Shell star.
HR 1052σ35BD+47 8432155238890124I 1167 03 30 34.5+47 59 434.36 K3III G:Mel 20 #900; Per OB3.
HR 1056BD+48 9382162038906 1173 03 31 29.4+49 12 356.29 A0Vn G:Mel 20 #934; Per OB3.,VAR:EA, amp. 0.1V, 5.363d.
HR 1059BD+48 9422166138912 03 31 49.1+49 24 036.39 B9III G:Mel 20 #954; Per OB3.
HR 1063BD+47 8472169938917 V396 Per03 32 08.6+48 01 255.47 B8IIIpMn G:Mel 20 #985; Per OB3.,S:Spectra show Mn. Helium weak. Si enhanced. Also classified B5Vp.,VAR:Alpha CV 5.45 - 5.53V, 2.4928d. First helium-weak star found to have periodic variations (1973).
HR 106936BD+45 77821770389242249 1182 03 32 26.3+46 03 255.31 F4III
HR 1072BD+44 7342180338927 KP Per03 32 39.1+44 51 206.41 B2IV G:Cas-Tau OB1.,VAR:Beta C 6.37 - 6.47V, 0.2101753d, multiple periods, 0.1982, 10.85, 0.01d.
HR 1074BD+34 67421856565311098 Var?03 32 40.0+35 27 425.90 B1V G:Per OB2.
HR 1078BD+39 81121912565382254 IW Per03 33 35.1+39 53 585.81 A5m SB:0.9171877d, K 99.3k/s, V0 +0.2k/s, asini 1.251.,VAR:Ell 5.80 - 5.85V, 0.9171877d.
HR 1087ψ37BD+47 8572219238980I Psi Per03 36 29.4+48 11 344.23 B5Ve vG:Mel 20 #1164; Per OB3; member of Pleiades group. Nonmember of Alpha Per cluster on basis of RV.,RV:Rotationally unstable shell star.,S:Shell star.,VAR:Amp. 0.04V, 0.5d. Hydrogen emission variable. Expanding circumstellar shell.
HR 1097BD+42 7952240238999 03 38 00.2+42 34 596.42 B8Vn
HR 1113BD+37 8112278056628 1225 03 41 07.9+37 34 485.57 B7Vne G:Member of the local association (Pleiades group).,VAR:Gamma Cas?, 5.55 - 5.58V.
HR 1122δ39BD+47 8762292839053131W Del Per03 42 55.5+47 47 153.01 B5IIIe t7.399.1C:Color excess E(B-V) = +0.04.,G:Per OB3.,S:C1 neutral carbon continuum shows discontinuities in UV. Lyman alpha observed from COPERNICUS.,VAR:Alpha CV? 2.98 - 3.03V, about 1d. Strong variable emission at 1650A, CaII?
HR 112340BD+33 69822951566462699 03 42 22.5+33 57 544.97 B0.5V 5.020.0C:Reddened star. Color excess E(B-V) = +0.24.,G:Per OB2.
HR 1127BD+48 9842304939063I2712 03 44 06.4+48 31 256.06 K4III 7.118.6C:Nicolet has 6.60V, Mermilliod 6.39V: no indication of variability.
HR 1130BD+45 80423139390712266 03 44 40.9+46 05 596.11 A7IV
HR 1131ο38BD+31 64223180566732726 Omi Per03 44 19.1+32 17 183.83 B1III 2.81.0C:Reddened star. Color excess E(B-V) = +0.32.,D:Binary. Combined mag., colors. Rotational velocity B, 150:k/s. Unresolved by speckle interferometry 1982.16.,DYN:0.005".,G:Per OB2 (not a member). Embedded in reflection nebulosity. In cluster IC 348.,M:In interstellar ultraviolet radiation field.,N:Atik; Ati; Al Atik.,P:Intrinsic polarization, probably due to circumstellar matter.,SB:4.4192d, K 109.3k/s, V0 +19.8k/s, msin3i 5.26, asini 6.63. Rotational velocity of secondary, 84k/s, primary,SB:85k/s.,VAR:Ell 3.79 - 3.85V, 4.419171d, possibly half.
HR 1133BD+36 74223193566752268 03 44 31.4+36 27 365.59 A2m
HR 1135ν41BD+42 8152323039078134I2738 1261 03 45 11.6+42 34 433.77 F5II 8.131.4
HR 1141BD+45 81123300390852746 03 45 59.3+45 40 555.66 B6V 8.46.5D:CPM.,G:Member of the local association (Pleiades group).
HR 1160BD+50 82523552242312769 03 48 18.3+50 44 126.14 B8Vne 6.27.0D:Probably optical.,S:Shell star.
HR 1163BD+33 71723625567092772 1305 03 47 52.6+33 36 006.57 B2.5V 4.03.2D:Binary.,G:Per OB2.,SB:ADS 2772A, 1.9406d, K 82k/s, V0 +20k/s, msin3i 0.883, asini 2.19.,VAR:B-A varies from 2.8 to 4.3V. Uncertain which component varies.
HR 1164BD+31 6502362656707 03 47 48.9+32 11 426.25 G0
HR 1170BD+43 8182372839128 V376 Per03 49 08.2+43 57 476.02 A9IV VAR:Delta Sct 5.8 - 5.91V, variable amp. Primary and beat periods, 0.098299 and 0.39206d.
HR 1176BD+44 8012383839134 Var?03 50 04.5+44 58 045.66 G2III+F2:V SB:vsini of secondary 85k/s. Unresolved by speckle interferometry 1983.93.,VAR:A variable comparison star was used when HR 1176 was suspected of variablility.
HR 117742BD+32 6672384856727 V467 Per03 49 32.6+33 05 295.11 A3V G:Per OB2.,SB:1.7653d, K 34.4k/s, V0 -11.9k/s, asini 0.832.,VAR:A published period, 22.58d, does not satisfy available SB observations, whereas the SB period does satisfy the,VAR:photometric equally well. However, more observations are badly needed.
HR 1191BD+33 7282413156761W 03 51 53.7+34 21 335.77 B1V 7.515.1G:Per OB2.
HR 1197BD+30 5822416756762 03 52 04.3+31 10 066.25 A5V G:Per OB2.
HR 1198BD+48 10152424039175 03 53 38.7+48 39 025.76 K0III
HR 1203ζ44BD+31 6662439856799144I2843 1397 03 54 07.9+31 53 012.85 B1Ib 6.512.9C:Reddened star. Color excess E(B-V) = +0.33.,D:AB CPM, B 9.16V B8IV; C, 9.12V at 33" optical; D, 10.35V, +0.713(B-V), +0.20(U-B), at 92" optical; E, 9.90V, A2V,,D:+0.33(B-V), +0.17(U-B), at 120" physical.,DYN:0.012".,G:IC 348; Per OB2.,RV:Comp. B +20.8k/s.,S:Interstellar CH detected optically. COPERNICUS data used to analyze the chemical abundances in line of sight to,S:Zeta Per: CO, HD, and OH. About 60% of the hydrogen in front of the star is molecular.,SB:1.765d, K 6.0k/s, V0 +22.2k/s.,VAR:2.80 - 2.93V.
HR 1207BD+47 91224504391952279 03 55 58.2+47 52 175.37 B6V G:Per OB3.
HR 1209BD+30 5912453456815I2859 X Per03 55 23.0+31 02 456.10 O9.5ep v5.822.5C:Heavily reddened.,D:CPM? Component A possibly optical counterpart or companion of X-ray source 4U0352+30. Possibly a triple system with a,D:neutron star moving around the optical primary in 22.4 hrs., and either apsidal period 581d or close double moving,D:around a distant component in 581d. Rotational velocity of primary, vsini 306k/s. Component ADS 2859B is normal M1III,,D:not T Tau type as once assumed.,G:May not be member of Per OB2; Zeta Per group.,M:Space velocities of X Per and Xi Per indicate the two stars approached to within 17 pc 2 million yrs ago.,P:Conflicting evidence whether observed polarization is intrinsic to the star or of interstellar origin.,S:Sp. data suggest occasional interruption of almost steady infall of material through rotating emission region by,S:outbursts of material from the star.,SB:580.7d, K 59k/s, V0 -50k/s, asini 471. Emission lines var. in RV, 22.4 hrs. and 581d.,VAR:ADS 2859A, Gamma Cas 6.07 - 7.0V, 580.7?d. Amp. about 0.02U. X-ray period 22.4 hrs. Spectrum variable. Sudden,VAR:decrease in H alpha emission followed by 450 sec. flare in continuum. Possible neutron star companion pulsating in,VAR:13.924 min. Simultaneous X-ray and optical obs. 21 Jan. 1975 showed X-ray var. by factor 2 but no corresponding optical,VAR:100 sec. quasi periodic photometric var. may indicate binary with compact companion undergoing mass accretion.
HR 121043BD+50 8602454624314IW 03 56 36.5+50 41 435.28 F5IV 4.875.3C:IR source in this direction corresponds to a Seyfert galaxy.,D:AB CPM. Component C, 11.4v at 101" optical. P, 12.5v at 279".,G:Hyades moving group.,SB:30.4380d, K 51.9k/s, V0 +25.1k/s, msin3i 0.910, asini 16.9; alternate orbit 30.4391d, K50.6k/s,,SB:msin3i 0.82, asini 15.53; vsini both components <17k/s.
HR 1215BD+34 7682464056824 1418 03 56 28.7+35 04 525.49 B1.5V G:Per OB2.,VAR:Beta C?, 5.45 - 5.50V. RV possibly var. 0.13169d.
HR 1220ε45BD+39 89524760568401472888 Eps Per03 57 51.2+40 00 372.89 B0.5V+A2V 5.18.8C:Color excess E(B-V) = +0.10.,D:AB CPM. B, 7.39V, -0.03(B-V), -0.52(U-B), B9.5V, vsini 300:k/s.,G:Cas-Tau OB1; member of Pleiades group.,VAR:Beta C, 2.88 - 3.00V, 0.216:d. Brightest component on visual triple. Photoelectric and spectroscopic resonant periods,VAR:found are submultiples of 26.9 hrs or 1.12d.
HR 1223BD+34 7732480956847 V386 Per03 58 03.1+34 48 526.53 A8V G:Per OB2.,SB:vsini both components 80k/s.,VAR:Delta Sct 6.50 - 6.58V, 0.052d.
HR 1226BD+38 8272484356849 03 58 29.1+38 50 256.30 gK1
HR 1228ξ46BD+35 7752491256856148I Xi Per03 58 57.9+35 47 284.04 O7.5III(n)((f)) eC:Color excess E(B-V) = +0.32.,G:Runaway star from Per OB2. Within 1d and exciting star of HII region S220. Ionizes region at edge of California nebula =,G:NGC 1499.,N:Menkib; Menkhib; Menchib.,S:Interstellar CO emission. Central Balmer emission in blue-violet only.,SB:6.951d.,VAR:Slightly variable, possibly same period as SB.
HR 1229BD+38 82924982568662910 03 59 40.0+38 49 146.38 R A1Vp: 2.71.5
HR 1234BD+36 8052515256899 04 01 14.7+36 59 246.41 A0V RV:Determinations of vsini range from 50 to 250k/s.
HR 1261λ47BD+49 110125642244121113 04 06 35.0+50 21 054.29 A0IVn
HR 127348BD+47 9392594039336152I MX Per04 08 39.7+47 42 454.04 B3Ve G:Per OB3; member of Pleiades group.,RV:Pole on.,S:Excess IR emission.,SB:16.934615d not confirmed.,VAR:Gamma Cas 4.00 - 4.10V, 55?d. Slow var. possibly associated with emission spectrum.
HR 127749BD+37 8812597557000 04 08 15.3+37 43 406.09 K1III
HR 127850BD+37 88225998570062297 04 08 36.6+38 02 235.51 F7V D:CPM with GC 4949 at 12' = ADS 2995, a triple system 7.3 dK2, 9.0 sep. 1"; C at 234".,G:Hyades group.
HR 1286BD+33 80726311570472300I 04 10 59.0+33 35 125.72 K1II-III
HR 1301BD+37 8972660557081 04 13 59.6+37 58 016.45 R G9III
HR 1303μ51BD+48 106326630394041117I3071 1518 04 14 53.9+48 24 344.14 G0Ib 6.083.8D:A* 4.13 G0Ib, 0.778y, a = 0.019". AB CPM; B, 11.8v at 15". C , 10.25V, +0.47(B-V), +0.06(U-B), B8.,SB:283.272d, K 20.7k/s, V0 +7.7k/s, asini 80.5. Unresolved by speckle interferometry.,VAR:ADS 3071A, 4.1 - 4.24V.
HR 130652BD+40 91226673394092306I 04 14 53.3+40 29 014.71 G5Ib+A2V SB:1576.44d, K 18.1k/s, V0 -4.5k/s, asini 358. Unresolved by speckle interferometry 1983.93. vsini of secondary,SB:100k/s.
HR 1324BD+49 11502696124531 b Per04 18 14.6+50 17 444.61 A2V G:In NGC 1545 #1; Hyades group.,M:Source of weak radio emission.,SB:Comp. ABC: 701.76d, K 11.4k/s, V0 +21k/s, asini 107. Comp. A: 1.527365d, K 39.4k/s, V0 var., asini 0.827.,SB:Unresolved by speckle interferometry.,VAR:Ell 4.59 - 4.65V, 1.527365d. Radio binary showing radio flare activity. Third component may eclipse primary.
HR 1328BD+41 8442702639447 04 18 08.2+42 08 286.22 B9V
HR 1330BD+49 11552708439457 04 19 13.3+50 02 565.45 A7V G:NGC 1545 #1.
HR 1333BD+50 97327192245442316 1550 04 20 11.5+50 55 155.55 B1.5IV G:Cas-Tau OB1.,SB:1.527365d, K 38.83k/s, V0 +20.66k/s, asini 0.815.,VAR:Amp. 0.020V.
HR 1337BD+41 8522727839468 04 20 14.4+41 48 295.92 K0III
HR 134354BD+34 8602734857171158IW 04 20 24.6+34 34 004.93 G8III 7.9110.0
HR 1344BD+31 7572734957166I 04 20 10.0+31 57 126.16 K5
HR 135053BD+46 87227396394832319 V469 Per04 21 33.2+46 29 564.85 B4IV G:Member of Pleiades group.,SB:Same period as VAR.,VAR:Amp. 0.01V, 7.29?hrs.
HR 1371BD+42 94627650395013172 04 23 35.9+42 25 416.23 A1pSi 0.50.4
HR 137755BD+33 8532777757212 04 24 29.2+34 07 505.73 B8V
HR 137956BD+33 85427786572163188 1592 04 24 37.4+33 57 355.76 F4V 3.64.9DYN:0.042".,VAR:ADS 3188B, 9.6 - 11.3v.
HR 1390BD+31 77627971572292325 04 26 06.3+31 26 205.28 K1III
HR 1419BD+32 8062845957269W 04 30 38.3+32 27 296.21 B9.5Vn D:Suspected of being double; probably single.
HR 1424BD+39 101328503572783273 A04 31 24.0+40 00 376.26 B8V 0.59.3D:CPM.
HR 143457BD+42 99028704396041124W 04 33 24.9+43 03 506.09 F0V 0.7116.2
HR 145458BD+40 100029094396392338IA 04 36 41.4+41 15 534.25 K4III+A3V 0.1D:A* 4.27 G8II+B, 28.67y, a = 0.054"(not confirmed).,S:Also classified K0II-III + B9V.,SB:10,470d, K 12.8k/s, V0 +5.9k/s, asini 1400. One of the longest SB periods known, 28.67y. Masses 6 and 5 solar.,SB:Unresolved by speckle interferometry. vsini of both components =<50k/s.
HR 1482BD+48 112829526396882347 04 41 24.1+48 18 035.67 A0V
HR 1489BD+37 95429645573772348 04 41 50.3+38 16 495.99 G0V
HR 1493BD+49 123029721397021128W 04 43 21.6+49 58 265.87 B9III 7.320.8
HR 149459BD+43 104329722396992349 04 42 54.3+43 21 545.29 A1Vn
HR 1500BD+40 10322986639715 04 44 12.9+40 47 136.08 B8IVne S:Shell star.
HR 1514BD+40 10453013839746 04 46 44.4+40 18 465.97 G9III
HR 1533BD+37 96930504574471133I 04 49 54.6+37 29 184.88 K3.5IIIBa0.2: N:Formerly 1 Aur, now in Perseus.

Revised+Historic NGC/IC, Version 22/9, © Dr. Wolfgang Steinicke [277]
Planetary Nebulae
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 65001 42 18.1+51 34 17PN12.210.13.12vB, p of D nebM 76, PK 130-10.1, CS=17.0, Little Dumbbell (SW)
IC 35103 47 33.0+35 02 50PN12.411.90.3Planetary = * 10m, * 9m p 14s, 2' sPK 159-15.1, CS=15.0
IC 200303 56 22.0+33 52 32PN12.611.40.33pB, eS, lE ns, * 13 n 4", * 12 sp 18"PK 161-14.1, CS=15.3
Galactic Nebulae
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 133303 29 18.0+31 25 00RN6 × 3F, L, * 10 nf (Auw No 17)LBN 741
NGC 149104 03 13.5+51 18 58EN25 × 25vB, S, iF, bM, r, * invLBN 704, in Sh2-206
NGC 149904 01 10.0+36 27 36EN5.0120 × 60vF, vL, E ns, difLBN 756, California nebula
NGC 157904 30 14.2+35 16 47RN12 × 8pB, vL, iR, mbM, * 8 350°, 2'LBN 766, Sh2-222
IC 206704 30 52.0+35 26 42ENvF, R, * 15 inv n, * 17 close npSS 20
Open Clusters
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 74401 58 33.0+55 28 24IV2p7.95Cl, pL, pRi, iF, st 11…13OCL 345
NGC 86902 19 04.0+57 08 06I3r5.318! Cl, vvL, vRi, st 7…14OCL 350, Chi Per, Double cluster
NGC 88402 22 05.0+57 07 48I3r6.118! Cl, vL, vRi, ruby * MOCL 353, Chi Per, Double cluster
NGC 95702 33 21.0+57 33 36III2p7.610Cl, pL, pRi, st 13…15OCL 362
NGC 103902 42 05.0+42 45 42II3m5.225Cl, B, vL, lC, sc st 9M 34, OCL 382
NGC 119303 05 55.0+44 23 00II3m12.63F, cL, erOCL 390
NGC 122003 11 40.6+53 20 53II2p11.82Cl, vS, st vFOCL 380
NGC 124503 14 41.4+47 14 19III1r8.410Cl, pL, Ri, C, iR, st 12…15OCL 389
NGC 134203 31 38.0+37 22 36III3p6.717Cl, vL, ab 60 stOCL 401
NGC 134803 34 06.0+51 25 12II2p6Cl, lRi, st LOCL 391
NGC 144403 49 25.0+52 39 18IV1p6.64Cl of ab 30 st 12…14OCL 394
NGC 149604 04 31.8+52 39 41II1p9.63Cl, segment of a ringOCL 396
NGC 151304 09 57.0+49 30 54II1m8.412Cl, L, vRi, pC, st vLOCL 398
NGC 152804 15 19.0+51 12 42II2m6.418Cl, B, vRi, cCOCL 397
NGC 154504 20 56.2+50 15 19II2p6.212Cl, pRi, lC, st LOCL 399
NGC 158204 31 39.0+43 44 36IV2p7.024Cl, vL, pRi, lC, st LOCL 407
NGC 160504 34 52.2+45 16 17III1m10.75Cl, vF, pS, C, st eSOCL 406
NGC 162404 40 36.4+50 27 42I2pn11.83F, cL, iF, 6 or 7 st + nebOCL 403, LBN 722, Ced 37, S 212
IC 34803 44 34.1+32 09 47IV2pn7.310pB, vL, vgbMIC 1985, OCL 409, LBN 758, CED 20
Galaxies
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 83203 11 05.4+35 23 11E213.912.91.6 × 1.3F, vS, * 9·10 spNGC 1226, UGC 2575, MCG 6-8-1, CGCG 525-2, CGCG 524-61
NGC 100102 39 12.6+41 40 18Sbc15.614.80.7 × 0.3vF, vSMCG 7-6-50, CGCG 539-69
NGC 100302 39 16.6+40 52 22Sc12.011.54.3 × 1.3pF, L, E 90° ±, mbM, rUGC 2137, MCG 7-6-51, CGCG 539-70, IRAS 02360+4039
NGC 100502 39 27.6+41 29 36E-S014.813.81 × 0.8vF, vSMCG 7-6-52, CGCG 539-71
NGC 102302 40 24.1+39 03 48E/SB010.49.47.4 × 2.5vB, vL, vmE, vvmbMUGC 2154, MCG 6-6-73, CGCG 523-83, Arp 135
NGC 1023 A02 40 36.9+39 03 37IBm14.313.61.3 × 0.7vB, vL, vmE, vvmbMArp 135
NGC 1040 102 43 12.5+41 30 01S013.912.91.7 × 0.8F, S, bMNGC 1053-1, UGC 2187, MCG 7-6-60, CGCG 539-83
NGC 1040 202 43 12.1+41 30 54S016.315.30.4 × 0.2F, S, bMNGC 1053-2, NPM1G +41.0081
NGC 105002 42 35.6+34 45 51SBa13.512.61.7 × 1.1F, S, * 18 inv nUGC 2178, MCG 6-6-78, CGCG 523-92, IRAS 02395+3433, KUG 0239+345, KARA 116, CGCG 524-1
NGC 105802 43 29.9+37 20 29Sc11.811.22.5 × 2.5pF, cL, R, glbMUGC 2193, MCG 6-7-1, CGCG 524-5, IRAS 02403+3707, CGCG 523-96, KUG 0240+371
NGC 1077 A02 46 00.6+40 05 24Sb14.413.61.1 × 0.8vF, pL, EUGC 2230, MCG 7-6-69, CGCG 539-95, IRAS 02428+3952
NGC 1077 B02 46 02.9+40 05 36SBb17.116.30.5 × 0.4vF, pL, EMCG 7-6-68, CGCG 539-95
NGC 108602 47 56.2+41 14 48Sc13.512.81.5 × 1vF, pS, D * nrUGC 2258, MCG 7-6-71, CGCG 539-101, IRAS 02447+4102
NGC 110602 50 40.5+41 40 20S013.312.31.3 × 1vF, vS, vF * att sUGC 2322, MCG 7-6-76, CGCG 539-112, IRAS 02474+4127
NGC 112302 52 51.2+42 12 19SBb12.912.11.8 × 1.3cF, S, iR, vgbM, rNGC 1122, UGC 2353, MCG 7-6-83, CGCG 539-117, IRAS 02496+4200
NGC 112902 54 27.3+41 34 47E313.512.42.9 × 2.1cF, pS, iR, vglbM, D or F * spUGC 2373, MCG 7-7-4, CGCG 539-124, VV 85, CGCG 540-6
NGC 113002 54 24.5+41 36 22C16.115.10.5 × 0.3eF, eSMCG 7-7-2, CGCG 539-122, CGCG 540-4
NGC 113102 54 34.0+41 33 33E015.614.60.4 × 0.4eF, eSMCG 7-7-5, CGCG 539-125, CGCG 540-7, 5ZW 286
NGC 113802 56 36.3+43 02 50SB013.812.81.1 × 1.1vF, vS, R, gbM, 2 S st ΔUGC 2408, MCG 7-7-12, CGCG 540-15
NGC 115903 00 46.4+43 09 46S014.513.50.5 × 0.4vF, S, R, vlbMUGC 2467, CGCG 540-23, IRAS 02575+4257
NGC 116003 01 13.2+44 57 20Scd13.512.81.5 × 0.7F, EUGC 2475, MCG 7-7-14, CGCG 540-27, KCPG 86A, IRAS 02579+4445
NGC 116103 01 14.1+44 53 51S012.111.02.8 × 2F, pS, lE, sbMUGC 2474, MCG 7-7-15, CGCG 540-26, KCPG 86B, IRAS 02579+4442
NGC 116403 01 59.8+42 35 08SBab13.913.11.3 × 1.1eF, vSUGC 2490, MCG 7-7-16, MK 1067, IRAS 02587+4223, CGCG 540-28, NPM1G +42.0105
NGC 116703 01 42.3+35 12 21S013.412.43.3 × 2.3vF, pL, R, spmbMUGC 2487, MCG 6-7-33, CGCG 524-45
NGC 116903 03 34.8+46 23 11SBb12.211.34 × 2.6pF, pS, iF, sbMUGC 2503, MCG 8-6-25, CGCG 554-20
NGC 117103 03 58.9+43 23 52Sc13.012.31.9 × 1vF, pL, iFUGC 2510, MCG 7-7-18, CGCG 540-31, IRAS 03006+4312
NGC 117503 04 32.3+42 20 25S0-a13.912.91.9 × 0.7F, cL, EUGC 2515, MCG 7-7-19, CGCG 540-32
NGC 117703 04 37.2+42 21 46S15.414.60.4 × 0.4vF, S, R, nf II 607IC 281, MCG 7-7-20, CGCG 540-33
NGC 118603 05 30.9+42 50 08SBbc12.211.43.2 × 1.2F * with neb appendagesNGC 1174, UGC 2521, MCG 7-7-21, CGCG 540-34, IRAS 03022+4238
NGC 119803 06 13.3+41 50 56E-S013.512.51.4 × 0.8Neb * 11IC 282, UGC 2533, MCG 7-7-24, CGCG 540-38
NGC 120703 08 15.4+38 22 56Sb13.512.72.3 × 1.6cF, vS, R, psb in npp endUGC 2548, MCG 6-7-43, CGCG 524-55, KCPG 87, IRAS 03050+3811
NGC 121203 09 42.3+40 53 35S0-a15.514.61 × 0.5eF, S, R, Algol nrIC 1883, UGC 2560
NGC 121303 09 17.3+38 38 57Sd15.014.41.8 × 1.4eF, lE, * close n, difficIC 1881, UGC 2557, MCG 6-7-45, CGCG 524-58
NGC 122403 11 13.5+41 21 48E-S015.014.01 × 0.8eF, vS, RUGC 2578, MCG 7-7-34, CGCG 540-55
NGC 122703 11 07.8+35 19 31SB0-a15.114.21 × 0.9vF, vSUGC 2577, CGCG 525-3, CGCG 524-62
NGC 123303 12 33.1+39 19 09Sb14.013.21.8 × 0.6F, vS, R, diffNGC 1235, UGC 2586, MCG 6-8-3, IRAS 03093+3907, CGCG 525-6, CGCG 524-65
NGC 125003 15 21.0+41 21 20S014.012.92.1 × 0.6vF, vS, RUGC 2613, MCG 7-7-40, CGCG 540-66
NGC 125903 17 17.3+41 23 08S015.314.30.7 × 0.7vF, S, R, vlbMMCG 7-7-46
NGC 126003 17 27.2+41 24 19S0-a14.213.31.1 × 0.5vF, S, RUGC 2634, MCG 7-7-47, CGCG 540-81, IRAS 03141+4113
NGC 126403 17 59.5+41 31 13SBab14.914.11 × 0.5vF, S, vlbMUGC 2643, MCG 7-7-50
NGC 126503 18 08.4+41 45 16E514.413.41 × 0.5vF, vS, mbMIC 312, UGC 2644, MCG 7-7-51, CGCG 540-86
NGC 126703 18 44.8+41 28 03E214.113.11.1 × 0.9F, vS, R, stellUGC 2657, MCG 7-7-55, CGCG 540-92
NGC 126803 18 45.2+41 29 21Sb14.213.40.9 × 0.6eF, S, lE, comUGC 2658, MCG 7-7-56, CGCG 540-93
NGC 127003 18 58.1+41 28 13E214.313.10.9 × 0.7vF, S, RUGC 2660, MCG 7-7-57, CGCG 540-95
NGC 127103 19 11.2+41 21 13SB0?14.913.90.5 × 0.2vF, vSCGCG 540-96
NGC 127203 19 21.3+41 29 26E112.911.82.2 × 2F, S, RUGC 2662, MCG 7-7-58, CGCG 540-98
NGC 127303 19 26.8+41 32 24S014.313.20.8 × 0.7vF, vSMCG 7-7-59, CGCG 540-99
NGC 127403 19 40.6+41 32 58E315.114.10.8 × 0.3vF, vSMCG 7-7-62, CGCG 540-102
NGC 127503 19 48.1+41 30 41S0/P12.611.92.3 × 1.6F, SUGC 2669, MCG 7-7-63, CGCG 540-103, 3C 84 , IRAS 03164+4119, Perseus A
NGC 127703 19 51.4+41 34 27S0-a14.713.60.8 × 0.3vF, vS, np II 603MCG 7-7-64, CGCG 540-104
NGC 127803 19 54.1+41 33 49E213.612.41.4 × 1.1pB, pS, R, bMIC 1907, UGC 2670, MCG 7-7-65, CGCG 540-105
NGC 127903 19 59.1+41 28 47S15.815.00.6 × 0.4vF, vSPGC 12449
NGC 128103 20 06.3+41 37 47E514.513.30.9 × 0.4vF, S, * 11 p 1'MCG 7-7-67, CGCG 540-108
NGC 128203 20 12.0+41 22 01E413.912.91.2 × 0.7vF, S, lbMNUGC 2675, MCG 7-7-68, CGCG 540-109
NGC 128303 20 15.5+41 23 55E114.713.60.7 × 0.6vF, S, vlbMUGC 2676, MCG 7-7-69, CGCG 540-110
NGC 129303 21 36.4+41 23 36E014.513.40.9 × 0.9vF, R, bM, np of 2MCG 7-7-75, CGCG 540-116, NPM1G +41.0114
NGC 129403 21 40.0+41 21 38E-S014.313.21.1 × 0.8vF, R, bM, sf of 2UGC 2694, MCG 7-7-76, CGCG 540-117, IRAS 03184+4111
NGC 133403 30 01.7+41 49 57Sbc14.013.21.5 × 0.7eF, pL, lbMUGC 2759, MCG 7-8-18, CGCG 541-17, IRAS 03266+4139
NGC 133503 30 19.4+41 34 24E-S014.813.81.1 × 0.6vF * in vF, eS nebUGC 2762, MCG 7-8-19, CGCG 541-18
NGC 146503 53 31.9+32 29 34S0-a14.613.71.7 × 0.5pF, pS, R, pB * nr pUGC 2891, MCG 5-10-3, CGCG 508-4
IC 25602 49 40.3+46 57 16C17.916.90.5 × 0.3cF, lE, S, 1st of 35ZW 280, no. 2 of 3 comps
IC 25702 49 45.2+46 58 32E-S013.812.61.4 × 0.8eF, pS, R, v diffic, 2nd of 3UGC 2298, MCG 8-6-11, CGCG 554-8
IC 25802 49 45.9+41 03 07SB0-a15.014.11 × 0.6vF, vlbM, * 9.5 f 2'UGC 2306, CGCG 539-107, KCPG 79B
IC 25902 49 40.8+41 03 20E-S015.314.30.7 × 0.6vF, double, dist 17"CGCG 539-106, NPM1G +40.0060, KCPG 79A
IC 26002 51 00.9+46 57 18E314.213.21 × 0.7eeF, pS, 2 F st nr, 3rd of 3UGC 2325, MCG 8-6-14, CGCG 554-11
IC 26202 51 43.2+42 49 42SB014.213.21.6 × 1.4eeF, pS, R, bet 2 st, v difficUGC 2335, MCG 7-6-80, CGCG 539-114
IC 26502 54 43.9+41 39 21E015.614.60.7 × 0.7eeF, eS, RMCG 7-7-6, CGCG 540-9, CGCG 539-127, NPM1G +41.0090
IC 26602 55 04.7+42 15 50S15.614.80.7 × 0.4eF, eS, RMCG 7-7-10, CGCG 539-130, CGCG 540-12
IC 275 103 00 55.7+44 21 01C M17.316.30.3 × 0.3eeF, pS, R, bet 2 st5ZW 309
IC 275 203 00 55.9+44 20 46C17.516.50.2 × 0.2eeF, pS, R, bet 2 st5ZW 309
IC 275 303 00 58.6+44 21 02C16.615.60.2 × 0.2eeF, pS, R, bet 2 st5ZW 309, NPM1G +44.0059
IC 27803 01 30.4+37 45 59E014.213.21.1 × 1.1vF, * 10 p 95", F * 12" spUGC 2481, MCG 6-7-32, CGCG 524-44
IC 28403 06 09.9+42 22 18Sd12.511.53.8 × 1.2eeF, pL, lE, D * np, bet 2 stUGC 2531, MCG 7-7-23, CGCG 540-37, IRAS 03029+4211
IC 28803 07 32.8+42 23 16S?15.114.21 × 0.3vF, vS, R, 2 st nf, ? S ClUGC 2544, MCG 7-7-27, CGCG 540-43
IC 29003 09 42.8+40 58 30Sb15.614.81.1 × 0.2eeF, S, RIC 1884, UGC 2561, CGCG 540-47
IC 29203 10 12.9+40 45 57Sd14.213.51.2 × 0.7eF, pS, R, * s, bet 2 stIC 1887, UGC 2567, MCG 7-7-30, CGCG 540-49, IRAS 03069+4034
IC 29303 10 56.1+41 08 16E-S015.314.30.6 × 0.4eF, S, RIC 1888, MCG 7-7-31, CGCG 540-53, NPM1G +40.0069
IC 29403 11 03.1+40 37 18SB0-a14.813.92.1 × 1.5vF, pS, irr RIC 295, IC 296, IC 1889, UGC 2574, MCG 7-7-33, CGCG 540-54
IC 29503 11 03.1+40 37 18SB0-a14.813.92.1 × 1.5eF, pS, RIC 294, IC 296, IC 1889, UGC 2574, MCG 7-7-33, CGCG 540-54
IC 30003 14 15.8+42 24 54S016.015.00.3 × 0.3eF, S, R, * 9 sp, np of 2
IC 30103 14 47.7+42 13 23E014.213.20.8 × 0.8eF, pS, R, sf of 2UGC 2606, MCG 7-7-36, CGCG 540-63
IC 30403 15 01.4+37 52 55Sb14.613.81.1 × 0.7vF, * 76" sf, np of 2UGC 2609, MCG 6-8-5, CGCG 525-10, IRAS 03118+3741
IC 30503 15 03.7+37 51 38E315.114.10.8 × 0.6vF, * 49" nfMCG 6-8-6, CGCG 525-12, NPM1G +37.0120
IC 30803 16 15.9+41 10 53S015.414.21.2 × 1.2eF, pS, iR, r ?UGC 2619
IC 30903 16 06.2+40 48 17S014.513.50.9 × 0.9eeF, pS, R, bet 2 stMCG 7-7-43, CGCG 540-72
IC 31003 16 43.0+41 19 29S013.912.71.1 × 1.1vF, pS, R, 1259 and 1260 nearUGC 2624, MCG 7-7-45, CGCG 540-75, IRAS 03135+4108
IC 31103 16 46.8+40 00 15S?15.014.10.9 × 0.6eF, pS, iR, bet 2 st, vF * v close fUGC 2625, CGCG 540-76
IC 31303 20 57.9+41 53 39E115.114.10.9 × 0.8eeF, vS, R, close D * nr sUGC 2682, MCG 7-7-73, CGCG 540-111
IC 316 103 21 19.9+41 55 43S M15.014.20.5 × 0.1eeF, pS, RMCG 7-7-74, CGCG 540-112
IC 316 203 21 19.9+41 55 55Sbc15.014.21.4 × 0.7eeF, pS, RUGC 2688, CGCG 540-112, IRAS 03179+4145
IC 32003 25 59.2+40 47 21SBab14.513.71.2 × 1.1eF, pS, R, vF * close pUGC 2732, MCG 7-8-7, CGCG 541-6
IC 187403 06 21.9+36 00 54SB0-a14.613.71 × 0.7F, vS, vlbM, difMCG 6-7-39, CGCG 524-50, NPM1G +35.0087
IC 190003 15 55.2+37 09 17S015.014.00.5 × 0.4F, S, pR, gbMNMCG 6-8-7, CGCG 525-13, NPM1G +36.0098
IC 190103 16 02.5+37 06 47Sa15.714.90.8 × 0.2F, vS, R, gbMNMCG 6-8-8, CGCG 525-14, NPM1G +36.0099
IC 190203 16 12.4+37 10 41S0-a15.514.60.4 × 0.4F, vS, R, sbM * 14CGCG 525-15, NPM1G +36.0100
IC 193403 31 13.9+42 47 34S015.014.01.2 × 0.5eF, pS, lbM, * 12 dist 34"UGC 2769
IC 200503 57 39.5+36 47 15S15.614.80.4 × 0.1F, vS, R, stellCGCG 526-15, "in" N 1499
IC 202704 06 39.6+37 06 57E015.114.10.4 × 0.4F, vS, R, vlbMUGC 2957, MCG 6-9-19

«Strasbourg-ESO Catalogue of Galactic Planetary Nebulae» Acker et al., 1992 [141]
PNGRA
J2000.0
Dec
J2000.0
Main IDPKIRASDiscovererIdentitiesoDiam
["]
rDiam
["]
Dist
[kpc]
Rvel
[km/s]
ExpVel
[km/s]
C* NameC* MagC* SP Type
PN G130.9-10.501 42 21+51 34 07NGC 650-51130-10.101391+5119CURTIS 1918ARO 2, M 76, VV 6, VV'9 67. 100. 1.2 -19.1 ± 1.2 38.5 (O-III), 40. (N-II)AG82 11
PN G133.1-08.601 58 49+52 53 44M 1- 2133-08.101555+5239MINKOWSKI 1946VV 8, ARO 116, VV' 11 18. : -12.1 ± 2.0 18.0 (O-III)AG82 13, CSI +52-01555 0, LS V +52 1, V741 PerB: 15.17, V: 13.44O + G2 Ib
PN G141.7-07.802 52 13+50 35 53A 5141-07.1ABELL 1955A55 4, ARO 206, VV' 14 127. 15. (N-II)AG82 16U: 20.6, B: 21.4, V: 21.4
PN G144.3-15.502 45 26+42 32 36A 4144-15.102421+4222ABELL 1964ARO 205, VV' 13 20. AG82 15B: 19.9
PN G147.4-02.303 41 43+52 17 01M 1- 4147-02.103379+5207MINKOWSKI 1946ARO 209, VV 11, VV' 17 4. 6.0 2.3 :-33.0 ± 3.9 13.0 (O-III)AG82 22V: 16.7
PN G149.4-09.203 27 15+45 24 20HDW 3HARTL et al 1983HaWe 4 540. AG82 20U: 16.0, B: 16.9, V: 17.0
PN G149.7-03.303 49 06+50 00 15IsWe 1ISHIDA et al 1987 780. -1.5 ± 0.5 5. (O-III)U: 15.71, B: 16.45, V: 16.56O(C)
PN G151.4+00.504 13 27+51 51 02K 3-64KOHOUTEK 1969 7.5
PN G153.7-01.404 15 55+48 49 41K 3-6504122+4842KOHOUTEK 1969 2. 5.
PN G156.9-13.303 45 27+37 48 48HaWe 5HARTL et al 1987 34. B: 17.1, V: 17.7
PN G159.0-15.103 47 33+35 02 49IC 351159-15.103443+3453BARNARD 1891ARO 19, VV 12, VV' 18 7. 7.0 -9.1 ± 1.4 15.0 (O-III)AG82 23B: 15.9, V: 15.8WR-Of
PN G160.5-00.504 46 43+44 28 01We 1- 2WEINBERGER 1977 92. AG82 36U: 20.37, B: 21.33, V: 20.87
PN G161.2-14.803 56 22+33 52 31IC 2003161-14.103531+3343HUBBLE 1920ARO 76, VV 15, VV' 21 8.6 9. -15.5 ± 2.2 21.5 (O-III)AG82 25B: 14.7, V: 15.0WC 7-8, WC early, O VI
PN G165.5-06.504 39 48+36 45 43K 3-6704364+3639KOHOUTEK 1969 0. 2.2 -77.0 ± 1.4 20.5 (O-III), 22.5 (N-II)AG82 34B: 18.5O(C)
PN G167.4-09.104 36 37+33 39 30K 3-6604333+3333KOHOUTEK 1969 0. 2.1 -67.5 ± 1.7 16.5 (O-III), 30.5 (N-II)AG82 32B: 16.26, V: 15.36Contin.

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