Sternbild Camelopardalis (Giraffe)

Camelopardalis
Camelopardalis: IAU Sternbildkarte [150]

Eigenschaften

Zwischen dem Sternbild Auriga und dem Polarstern klafft am Firmament eine Stelle gähnender Leere. Nur wenige Sterne erreichen eine Helligkeit, die unser Auge fesseln und zu einer Assoziation verleiten würde. Gerade mal zwei Sterne sind mit bloßem Auge gut sichtbar. Die Fläche des Sternbilds beträgt 757 Quadratgrad und das Zentrum kulminiert jeweils etwa am 23. Dezember um Mitternacht. [9, 15]

Daten für das Sternbild Camelopardalis [150]
IAU NameCamelopardalis
IAU GenitivCamelopardalis
IAU KürzelCam
Deutscher NameGiraffe
Saison (47° N)September … März
Rektaszension03h 15m 36s … 14h 27m 08s
Deklination+52° 39' 56" … +86° 05' 51"
Fläche757 deg2
Nachbarn (N↻)UMi, Cep, Cas, Per, Aur, Lyn, UMa, Dra

Deep-Sky Objektbeschreibungen

Sternbild Camelopardalus
Sternbild Camelopardalus: Illustration aus «Prodromus Astronomiae» von Johannes Hevelius, 1690. Spiegelverkehrte Ansicht von «außerhalb der Himmelssphäre» [19]

Geschichte

Die Giraffe wurde erst zu Beginn des 17. Jahrhunderts in die Sternbilderkunde eingeführt und hat somit keinen mythologischen Hintergrund. Das Sternbild wird meist dem holländischen Astronomen Petrus Plancius zugeschrieben, doch hat der Mathematiker Jakob Bartsch, ein Schwiegersohn Johannes Kepler, es bereits 1624 in einem Buch erwähnt. Dieser jeder dichterischen Phantasie bare Mathematiker taufte in seinem Werk Usus astronomicus planisphaerium Argentinae diese amorphe Stelle am Himmel auf den Namen "Giraffe". Die Giraffe war im antiken Griechenland unter dem Begriff "Leoparden-Kamel" bekannt. Jakob Bartsch zog es vor, das Sternbild als Kamel zu bezeichnen, namentlich das Kamel, welches Rebekka von Haran nach Kanaan brachte um Isaak zu heiraten. (Genesis 24:61). Weitere von Bartsch benannte Sternbilder sind Columba und Monoceros. Da die Astronomen ungern einmal eingebürgerte Sternbildnamen ändern, blieb Camelopardalis (auch Camelopardus) bis auf den heutigen Tag erhalten. [7, 21, 133]

Kataloge

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 967BD+65 33820104126862436 03 17 31.6+65 39 316.36 A3V 0.40.5D:AB 6.8 A2V, 7.3 A4V, 330y, a = 0.386". Combined mag., colors.,RV:Discordant sign from only two available sources, -7.5, +6.4.
HR 985BD+65 3402033612704W BK Cam03 19 59.4+65 39 084.84 B2.5Ven v7.7120.9D:Probably optical.,G:Cas-Tau OB1.,S:Shell star.,SB:4.5y.,VAR:Gamma Cas, 4.78 - 4.89V. Spectrum var. 4.5y from 1916 to 1931, previously longer cycles, but no changes noted after,VAR:1937. R-I also found at -0.03 and -0.05.
HR 1009BD+64 39120797127431096I 1121 03 24 40.5+64 35 105.23 M0II
HR 1033BD+59 65721203127702538 03 28 23.6+60 15 206.49 B9V+A1 1.00.2D:AB 6.8 B9V, 7.8 A1V, 259.90y, a = 0.370". Combined mag., colors.
HR 1035BD+59 66021291240541222544 1152 03 29 04.1+59 56 254.21 B9Ia 4.32.4G:Cam OB1; in reflection nebula; member assoc. Cam R1 at 870 pc.,VAR:H alpha profile var.
HR 1040BD+58 6072138924061I 03 29 54.9+58 52 434.54 A0Ia eG:Cam OB1; in reflection nebula; member assoc. Cam R1 at 870 pc.,VAR:H alpha profile variable.
HR 1043BD+58 60821427240622563 1158 03 30 11.3+59 21 586.13 A2V 1.42.5
HR 1046BD+54 68421447240642565 1159 03 30 00.2+55 27 075.09 A1V 4.814.8D:AB CPM.,G:UMa stream. Possible Eggen group with HR 63, q.v.,VAR:Delta Sct.
HR 1068BD+58 61921769240932592 A03 33 32.1+58 45 546.40 A4III 1.720.4D:AB CPM. B, spectral class F2V. Component C, 10.5v at 164".,S:Also classified Am(A3/A7/F0).
HR 1071BD+57 73021794240982252 03 33 41.2+57 52 086.37 F7V
HR 1073BD+54 6932181924099 03 33 39.0+54 58 295.98 A3V
HR 1077BD+59 67521903241112612 03 35 00.8+60 02 286.46 F3V 0.91.1D:AB 6.8 F3V, 7.6 F9V, 287.7y, a = 1.245". Combined mag., colors. Mass AB, 2.2 solar. C, 10.3v at 92" optical.
HR 1094BD+56 8262231624133 03 38 19.7+56 55 586.30 B9p vVAR:Spectrum variable.
HR 1105BD+62 5972264912874129I BD Cam03 42 09.3+63 13 005.10 S3.5/2 S:Technetium not abundant, as previously reported.,VAR:Lb 5.04 - 5.17V, 6.7 - 6.85p.
HR 1112BD+59 6992276424169I2691 03 42 42.7+59 58 105.76 K3IIb 2.454.7D:Component D, 8.73V, +0.10(B-V), -0.22(U-B), B8III.,S:Spectrum formerly classified as K4Ib. According to P. C. Keenan (October 1986), recent spectrograms, although not of,S:extremely high quality, show that star is not as luminous as Ib, with best spectral type of S. Yorka and P. C.,S:Keenan reported as K3IIb, although it may be slightly later.
HR 1124BD+66 28423005128902267 03 46 00.9+67 12 065.80 F0IV
HR 1129BD+62 6042308912891IS 03 46 02.3+63 20 424.80 G0III+A3V 1.00.1D:5y? Sep. 0.052". vsini of secondary =<50k/s.,S:Also classified G2II-III + B9V.,SB:219.971d, K 39.15k/s, V0 -18.38k/s, asini 118.
HR 1138BD+70 257232775000 03 49 13.8+70 52 165.44 A2m SB:15.5132d, K 22.2k/s, V0 +16.0k/s, msin3i 0.0813, asini 4.62. vsini both components 25k/s.
HR 1147BD+55 8242338324215 03 47 32.2+55 55 216.10 B9Vnn
HR 1148γBD+70 259234015006138W 03 50 21.5+71 19 564.63 A2IVn 3.9106.3
HR 1155BD+65 3692347512916I BE Cam03 49 31.2+65 31 344.47 M2+IIab eC:Large infrared excess.,G:In reflection nebula.,S:Ultraviolet FeII emission.,VAR:Lc 4.35 - 4.48V, amp. 0.12p.
HR 1158BD+62 6122352312917 03 49 36.7+63 17 505.85 A5Vn
HR 1161BD+56 8462359424244W 03 49 19.6+57 07 056.46 A0Vn 0.858.3
HR 1166BD+68 2862366212929 03 51 41.8+68 30 276.32 B9IVp
HR 1192BD+57 75224141242761105 03 53 43.3+57 58 305.80 A5m
HR 1196BD+71 2222416450402277 03 56 30.2+71 49 186.34 A5m
HR 1204BD+62 62824479129692281 03 57 25.5+63 04 205.03 B9.5V e
HR 1205BD+60 7682448012968I2867 03 57 08.3+61 06 325.00 K3I-II+A3V: 3.21.7D:Companion A0, CPM.,DYN:0.003".
HR 1241BD+68 30325274130062291I 04 06 03.1+68 40 485.87 K2III
HR 1242BD+58 69025291243842290 04 04 27.2+59 09 205.06 F0II
HR 1248BD+65 3912542513015 04 06 39.0+65 31 156.17 A3m
HR 1255BD+53 7322560224411 04 06 36.6+54 00 316.31 K0III-IV
HR 1260BD+61 67625638130312984 ASZ Cam04 07 51.1+62 19 486.99 B0III 0.317.9D:AB fixed. Some confusion in literature as to which component is A, which B. SZ CAM is Np = B, 6.94V, +0.41(B-V),,D:-0.53(U-B), O9.5V, vsini 160:k/s. Colors of both components have been described as "yellowish" even though both have,D:B-type spectra. Component Q, 10.39V, +0.58(B-V), -0.26(U-B).,G:Open cluster NGC 1502 #1, near center and probable member of cluster.,S:Luminosity of A variously classified II-III, V. Component B classified O9.5V, B0III or B0IIn.,SB:ADS 2984B, same period as for variable light. K 110.9k/s, V0 -22.8, asini 4.11.,VAR:Two variables: ADS 2984A = NSV 1458, amp. 0.05V, SB; component B = SZ Cam, Np, EA 7.0 - 7.29B, changing period, abrupt,VAR:change in 1972 from 2.6984378 to 2.69854365, later to 2.6985439d.
HR 1270BD+59 7592587724436 04 09 27.6+59 54 296.28 G8IIa
HR 1276BD+54 7402594824440 04 09 22.4+54 49 446.18 R F5V
HR 1281BD+71 239260765125 04 13 44.9+72 07 356.03 K1III
HR 1282BD+68 3102610113061 04 12 51.6+68 30 066.32 K0
HR 1296BD+57 78526553244952304 Var?04 15 01.8+57 27 376.08 A4III VAR:Probably var., amp. 0.08V.
HR 1305BD+61 6872667013075 04 16 53.6+61 51 015.70 B5Vn
HR 1313BD+57 7872675524514 04 17 08.2+57 51 385.71 K1III
HR 1314BD+53 75026764245122310 04 16 43.1+53 36 435.19 A2Vn
HR 1327BD+64 43327022130982315 04 20 40.3+65 08 265.27 G5IIb G:In Ursa cluster; Sirius group; UMa stream.
HR 1335BD+60 80027245131132317I 1558 04 21 47.6+60 44 085.39 M0III
HR 1342BD+56 9052732224563 04 21 51.8+56 30 245.88 R A3V
HR 1352BD+59 79327402245773146 1566 04 22 57.9+59 36 596.19 A4V 3.132.3VAR:ADS 3146B, 10.5 - >12V.
HR 1382BD+57 800278552461523243203 04 27 00.9+57 35 076.32 A0III 5.920.6D:Optical.
HR 1401BD+72 22728204523823333267 04 33 30.7+72 31 435.94 A8m 6.626.0G:Hyades group.,SB:4.195d, K 31.3k/s, V0 +9.0k/s, asini 1.81.
HR 14171BD+53 77928446246721653274 AVar?04 32 01.8+53 54 395.77 B0III 1.110.3D:AB binary. B, 6.94V, +0.16(B-V), -0.70(U-B), B1IV? vsini =<25k/s.,G:Cam OB1.
HR 1440BD+63 51528780131962336 04 36 24.2+64 15 425.94 A1V
HR 14662BD+53 79429316247443358 04 39 58.1+53 28 235.35 A8V 1.60.3D:AB 5.8 F0V, 7.4 F9V, 26.25y, a = 0.18" or 26.797y, a = 0.157". ABxC 5.6, 7.3, 425.0y, a = 1.38". Component D, 13.2v at,D:at 24" optical. Spectral classes component A, A9V; B, F8V; C, F8V.,DYN:0.004".
HR 14673BD+52 8652931724743I3359 1681 04 39 54.7+53 04 475.05 K0III 7.03.8SB:121d, K 28.2k/s, V0 -40.5k/s, asini 46.9.,VAR:ADS 3359A, Cep?, 5.05 - 5.10V, 5d?
HR 1468BD+76 174293295289 04 46 00.3+76 36 406.49 F7V
HR 1486BD+59 82629606247773391 04 43 18.1+59 31 156.50 R A7IV 0.00.1D:280.0y, e 0.56, a 0.45", i 51.9d, mag. diff 0.0.
HR 1491BD+75 189296785309173W 04 48 50.3+75 56 286.06 A9IV 6.096.9
HR 1510BD+70 3223008553262358 04 50 36.4+70 56 306.37 A0IV
HR 15114BD+56 97330121248291753432 04 48 00.3+56 45 265.30 A3m 7.599.0G:Hyades group.,S:Also classified A8IVbmvs.
HR 1515BD+55 9283014424834 04 48 07.0+55 36 096.26 R F0 G:Hyades group.
HR 1527BD+63 54330442132912362IW 04 52 05.2+63 30 195.44 M3IIIab 4.5115.4G:Eta Cep group.
HR 1542α9BD+66 3583061413298178 04 54 03.0+66 20 344.29 O9.5Ia eC:Color excess E(B-V) = +0.32.,G:In cluster NGC 1502. A possible runaway star from Cam OB1; in reflection nebula. Member assoc. Cam R1 at 870 pc.,S:H alpha emission due to extended envelope. uv 1548 absorption strong, 1394 very strong. Central Balmer emission in,S:blue-violet only.
HR 1546BD+52 8913075224894 04 53 09.8+52 50 276.41 A2V
HR 15555BD+55 941309582490423673508 04 55 03.1+55 15 335.52 B9.5V 6.412.9D:CPM.
HR 1561BD+52 8983113424919 04 56 07.1+52 52 105.75 A2V s
HR 15687BD+53 82931278249293536 04 57 17.2+53 45 084.47 A1V 3.40.4D:AB 4.5, 7.8, 284.0y, a = 0.78". C, 11v at 26" CPM, possibly physical.,G:UMa stream.,SB:ADS 3536A, 3.8845d, K 35.8k/s, V0 -9.5k/s, asini 1.91.
HR 1572BD+74 229313125385I 05 02 20.1+74 16 096.06 K5III
HR 1587BD+73 264315635403I 05 04 13.0+73 45 506.66 R K0
HR 15888BD+52 9063157924943I 04 59 46.3+53 09 206.08 K4III
HR 1589BD+73 265315905407W 05 04 39.8+74 04 015.96 R A1V 1.00.6D:136.0y, e 0.32, a 0.425", i 88d, mag. diff 1.0.
HR 1593BD+60 85331662133413590 05 01 35.9+61 04 416.03 F4V 5.55.4D:CPM.
HR 1594BD+66 3703167513344 05 02 50.4+66 49 226.19 dF6 G:Hyades group.
HR 1603β10BD+60 8563191013351182I3615 A05 03 25.1+60 26 324.03 G1Ib-IIa 3.480.8C:Color excess E(B-V) = +0.16.,G:Group with HR 1622 and 1719, all nearly same proper motion.
HR 162211BD+58 8043234325001W BV Cam05 06 08.5+58 58 215.08 B2.5Ve 1.0180.5D:Optical pair with HR 1623.,G:Group with HR 1603, 1719.,RV:Pole on. Rotationally unstable Be shell star.,VAR:Gamma Cas, amp. 0.07V, period a few hours?
HR 162312BD+58 8053235725003W BM Cam05 06 12.2+59 01 166.08 K0III 1.0180.5D:Optical pair with HR 1622; C, 10.8v at 173" from B; D, 13.3 at 16" from B.,SB:80.1745d, K 22.7k/s, V0 +0.6k/s, asini 23.4.,VAR:RS CVn amp. 0.14V, 82.8d.
HR 1624BD+60 8573235613369I 05 06 29.7+61 10 126.04 K5II
HR 1630BD+54 85932445250073667 05 06 22.0+54 24 217.24 R G5 3.76.7M:HR mag. 6.31 should have been 7.31.
HR 1636BD+69 30232518133822382 05 09 36.7+69 38 226.41 K1III
HR 1643BD+73 2743265054552387 BN Cam05 12 22.4+73 56 485.43 B9pSi RV:At times variable in period 7.993d.,VAR:Alpha CV, amp. 0.10U, 0.06B, 0.05V, 0.7325d.
HR 1647BD+64 50032715133882384 05 09 44.5+64 55 106.41 F6V
HR 1650BD+76 1903278154643738 1854 05 14 35.6+76 28 226.37 A0V 4.51.5VAR:ADS 3738B, amp. 1.8v?
HR 1675BD+61 7663326613409 05 13 03.2+61 51 006.17 A2III
HR 167814BD+62 7343329613413 05 13 31.3+62 41 296.50 A7Vn
HR 1683BD+73 280335415483 05 18 13.3+73 16 055.74 R A0V
HR 1686BD+79 1693356454961913864 A05 22 33.5+79 13 525.05 F6V 3.710.4D:B, dF5, optical. C observed only once.
HR 1688BD+59 8573361825088 05 15 11.3+59 24 206.15 K2III-IV
HR 171915BD+57 8743423325125 05 19 27.8+58 07 026.13 B5V G:Group with HR 1603, 1622. Cas-Tau OB1.
HR 1720BD+62 74234255134602397I 05 20 22.6+62 39 135.61 K4I:
HR 1745BD+77 1953465355352404 05 29 25.7+77 58 396.56 A7III
HR 175116BD+57 87934787251612402W 05 23 27.8+57 32 405.28 A0Vn 7.7106.2
HR 180217BD+62 7593558313518203I 2003 05 30 10.2+63 04 025.42 M1IIIa
HR 182818BD+57 88936066252411150 2058 05 32 33.8+57 13 166.48 F8V
HR 1844BD+74 252363845593205I 2337 05 39 43.7+75 02 386.17 M0III
HR 1853BD+66 4013649613548W 05 37 16.2+66 41 466.26 A8Vn 0.80.3
HR 185719BD+64 53636570135504177 05 37 15.1+64 09 176.15 A0V 4.01.6D:CPM.
HR 1916BD+65 48537289135702426I 05 42 26.4+65 41 525.60 gK5
HR 194124BD+56 10503760125333 05 43 01.6+56 34 546.05 K0III
HR 194323BD+61 8163763813590 05 44 08.6+61 28 366.15 gG5
HR 196926BD+56 10583809125362 2615 05 46 30.4+56 06 565.94 A4Vn
HR 1976BD+62 78438284136184376 05 49 04.9+62 48 296.13 R A4V 0.90.9
HR 199229BD+56 106538618254034412 05 50 34.0+56 55 086.54 A4IV-V 4.225.1D:Third component mag. diff 6.29V, 80" from A.
HR 1994BD+68 41238645136352438 05 52 55.5+68 28 176.20 G9III
HR 200630BD+58 8633883125419 05 52 17.4+58 57 516.14 A0V s
HR 202731BD+59 92039220254472446 TU Cam05 54 57.8+59 53 185.20 A2V SB:2.9333d, K 78.0k/s, V0 -4.0k/s, asini 3.15.,VAR:EB 5.12 - 5.29V, 2.933241d.
HR 2041BD+66 41339429136622448 05 57 35.0+66 05 466.25 K0
HR 2078BD+75 2474005557302459 06 05 09.3+75 35 096.40 R K5
HR 2121BD+59 9374082725551 06 05 08.3+59 23 356.34 K1III-IV G:Probable Hyades group.
HR 2126BD+63 6304095613715 06 06 39.2+63 27 136.39 R K0
HR 215237BD+58 8974159725597I 06 09 59.1+58 56 095.36 G8III
HR 216536BD+65 5174192713756233I 06 12 51.1+65 43 065.32 K1.5IIIbCN-0.5
HR 220140BD+60 9384263313772IW 06 15 40.6+59 59 575.35 K3III 5.1102.7
HR 2209BD+69 3714281813788234 06 18 50.8+69 19 114.80 A0Vn
HR 2285BD+70 4014447258615039 06 28 14.6+70 32 085.97 R A4V 5.95.7D:CPM.
HR 2346BD+79 208455605911 06 40 16.8+79 35 586.54 R A1V
HR 2350BD+82 1774561810433950 06 44 30.2+82 06 556.65 A5V
HR 2363BD+78 2274586659192507I 06 40 28.8+77 59 455.73 gK5
HR 2365BD+73 3404594759092503 06 37 54.9+73 41 446.24 F2
HR 2396BD+71 3594650959252511 06 40 32.2+71 44 565.92 K0III
HR 2401BD+79 212465885946248 06 46 14.1+79 33 535.45 F8V SB:60.0d, K 1.7k/s, V0 +16.2k/s, asini 1.245. Orbit questioned by Morbey and Griffin (1987, ApJ, 317, 343).,SB:Unresolved by speckle interferometry.
HR 249042BD+67 45448879139732523 06 50 57.1+67 34 195.14 B4IV
HR 251143BD+69 3944934013986259 06 53 42.2+68 53 185.12 B7III
HR 2527BD+77 266498786022260I 07 00 04.0+76 58 394.55 K4III G:Wolf 630 group.
HR 2581BD+70 430508856041IW 07 01 21.5+70 48 295.68 gK4 5.3117.0
HR 2617BD+70 432520306074I 07 05 51.8+70 43 556.50 R K0III
HR 2681BD+72 3525407061152552 07 13 58.1+71 49 006.35 K0
HR 2709BD+81 242550751164 07 25 21.9+81 15 276.31 A0III
HR 2742BD+82 2015596611793951I VZ Cam07 31 04.4+82 24 414.96 M4IIIa G:Hyades group.,VAR:SR 4.80 - 4.96V, 6.40 - 6.70p, 23.7d.
HR 277247BD+60 104856820262985995 07 22 17.2+59 54 076.35 A8m 4.52.2
HR 2797BD+81 252575081194 07 34 39.7+80 53 486.41 R gG7
HR 2809BD+66 50257742141952571 07 27 25.8+66 19 546.47 B9III
HR 2830BD+68 4805842514211284I 07 30 52.7+68 27 565.64 gK2
HR 297551BD+65 59362066143212602 07 46 40.1+65 27 215.92 gK2
HR 297749BD+63 7336214014322 BC Cam07 46 27.4+62 49 506.49 F0pSrEu VAR:Alpha CV 6.43 - 6.48V, 4.285d. Magnetic field same period.
HR 2997BD+80 238626131254 07 56 17.3+80 15 566.56 G8V
HR 3075BD+74 338643076378300I 08 00 11.7+73 55 055.41 K3III
HR 3082BD+79 2656448663922617W 08 04 47.1+79 28 475.42 A0pSi 8.36.7S:Magnetic star.
HR 3108BD+84 1696529913001639 08 16 53.8+84 03 286.49 A3IV
HR 310953BD+60 11056533914402302S AX Cam08 01 42.4+60 19 286.01 A2pSrCrEu vRV:1.14229d, 8d, and order of years. Possibly binary.,SB:2380d, K about 8k/s, V0 -2.2k/s, asini 220.,VAR:Alpha CV 5.95 - 6.08V, 8.0278d. 1.14d also possible. Length of period varies in cycles 1.8 yrs. Magnetic and,VAR:spectrum variable 8.0269d; also rotation period.
HR 3112BD+63 74965448144072619W 08 02 30.8+63 05 256.40 G1III 2.448.6
HR 3197BD+82 2356793413193952 08 24 32.9+82 25 516.32 A2Vn
HR 3216BD+76 310683756487310 08 19 32.2+75 45 255.54 G8III
HR 3352BD+75 3427197365926872 4133 08 36 48.7+74 43 256.31 A2m 3.51.8D:CPM.,SB:ADS 6872A, 4.285d, K 63.5k/s, V0 -7.4k/s, asini 3.72.,VAR:ADS 6872B, L 9.0 - >12v.
HR 3379BD+74 370725826605322 08 39 42.6+73 37 476.15 G7III
HR 3581BD+84 1967699014611640 09 15 21.2+84 10 526.33 F2III
HR 3666BD+74 393795176816 09 19 55.8+74 00 596.50 R G8III
HR 3934BD+84 2258632116373955 Var10 08 34.3+83 55 066.37 K0 VAR:Amp. 0.13V.
HR 4062BD+84 234895711701 10 29 41.5+84 15 085.50 F0IV G:Hyades group.
HR 4084BD+83 297900891714911 4864 10 31 04.6+82 33 315.26 F2V
HR 4429BD+81 3739994518843956 5230 11 31 50.4+81 07 386.15 A2m
HR 4586BD+81 38910421619673957I 5415 12 00 18.6+80 51 116.17 M2III G:61 Cyg group.
HR 4606BD+86 17610490419751642 12 04 28.1+85 35 146.27 F6V
HR 4609BD+77 4611049857500451 12 05 15.1+76 54 215.80 G9III
HR 4639BD+82 3561059431991W 12 11 00.0+81 42 366.00 gK5 2.066.7
HR 4646BD+78 4121061127522454 12 12 11.9+77 36 595.14 A5m SB:1.2710d, K 63.2?k/s, V0 +0.3k/s, asini 1.10.
HR 4852BD+81 40211111220803017 12 44 26.0+80 37 166.40 A5m S:Also classified A5V, A6III.
HR 4892BD+84 28911201421018682 B12 49 06.6+83 25 055.85 A0V+A2V 0.521.6D:CPM with HR 4893.,N:With HR 4893 called 32 Cam in Hevelius and some later catalogues. NOT Flamsteed 32. In BAC the two are listed as in UMi.,N:Fl. 32 Cam = 30 Aur = HR 2029.,SB:ADS 8682B, 3.2866d, K 108.3k/s, V0 -0.1k/s, msin3i 2.47, asini 4.89. vsini both components 17k/s.
HR 4893BD+84 29011202821028682 A12 49 13.6+83 24 465.28 A1IIIShell 0.521.6D:CPM with HR 4892.,N:See HR 4892.
HR 5009BD+81 41611533721643056W 6153 13 12 25.4+80 28 176.25 K0Ib 4.01.1S:Also classified G8III + A8V:.,VAR:Fainter component 8.5 - 10.5v.
HR 5091BD+79 42211756678213075 13 26 56.7+78 38 385.77 G2.5IIIbCH1
HR 5131BD+77 5161186867848I 13 34 42.8+76 32 486.57 R K5III:
HR 5203BD+83 39712056522661643 13 42 23.1+82 45 095.98 G9III

Revised+Historic NGC/IC, Version 22/9, © Dr. Wolfgang Steinicke [277]
Planetarische Nebel
NameRADecTypbMagvMagDimDreyer BeschreibungIdentifikation, Anmerkungen
NGC 150104 06 59.4+60 55 17PN13.311.50.87planetary, pB, pS, vlE, 1' diamPK 144+6.1, CS=14.4
IC 356812 33 06.9+82 33 51PN11.610.60.17Planetary or neb * 9.5, * 13 p 15"PK 123+34.1, UGC 7731, CS=11.4
Offene Sternhaufen
NameRADecTypbMagvMagDimDreyer BeschreibungIdentifikation, Anmerkungen
NGC 150204 07 49.2+62 19 54II3p6.920Cl, pRi, cC, iFOCL 383
NGC 170805 03 27.0+52 50 00OCL20Cl, vL, pRi, lC, st L and S
IC 36104 18 50.6+58 14 58II1r11.77F, L, ? neb ClOCL 393
Galaxien
NameRADecTypbMagvMagDimDreyer BeschreibungIdentifikation, Anmerkungen
NGC 146904 00 27.8+68 34 39E-S013.712.71.9 × 0.8vF, vS, R, B * nrUGC 2909, MCG 11-5-4, CGCG 305-3
NGC 148504 05 03.4+70 59 48Sb13.412.62.1 × 0.7eF, pS, RUGC 2933, MCG 12-4-10, CGCG 327-14, IRAS 03598+7051
NGC 153004 23 26.9+75 17 40SBb12.311.54.4 × 2.5pB, LUGC 3013, MCG 13-4-4, CGCG 327-17, IRAS 04170+7510, KUG 0417+751, 7ZW 12, KARA 147, CGCG 347-4
NGC 156004 32 47.5+71 52 46Scd12.211.49.8 × 1.5vF, L, E, * 9.3 spUGC 3060, MCG 12-5-5, CGCG 328-6, FGC 71A
NGC 156904 30 49.1+64 50 53IBm11.911.03.7 × 1.8pB, S, lE, bNM, * 9.5 n 1'UGC 3056, MCG 11-6-1, CGCG 306-1, Arp 210, 7ZW 16, IRAS 04260+6444
NGC 157304 35 04.2+73 15 47E312.811.71.9 × 1.3vF, S, * 9.5 fUGC 3077, MCG 12-5-8, CGCG 328-9, 7ZW 18
NGC 1573 A04 48 26.7+73 28 10SBbc14.814.01.6 × 1.3vF, S, * 9.5 fUGC 3150, MCG 12-5-20, CGCG 328-21, IRAS 04423+7322
NGC 196105 42 03.9+69 22 43SBbc11.711.04.5 × 3.1cF, pL, iF, mbM, er, * inv (? PD)IC 2133, UGC 3334, MCG 12-6-7, IRAS 05365+6921, CGCG 329-8, Arp 184
NGC 212806 04 34.0+57 37 39E-S013.612.61.5 × 1.1vF, vS, vlEUGC 3392, MCG 10-9-10, CGCG 284-6, IRAS 06002+5737
NGC 214606 18 38.3+78 21 21SBab/P11.410.65.4 × 2.9pB, 2' l, lEUGC 3429, MCG 13-5-22, CGCG 348-17, KCPG 110A, IRAS 06106+7822
NGC 2146 A06 23 54.6+78 31 48SBc13.512.93 × 1.2pB, 2' l, lEUGC 3439, MCG 13-5-25, CGCG 348-19, IRAS 06155+7833, KUG 0615+785, KCPG 110B
NGC 225606 47 14.2+74 14 13E/SB013.512.52.3 × 2F, R, * 9.5 3' sfUGC 3519, MCG 12-7-15, CGCG 330-14
NGC 225806 47 46.5+74 28 53S013.011.92.3 × 1.5F, 2 st 10·11 fUGC 3523, MCG 12-7-16, CGCG 330-15
NGC 226807 14 17.5+84 22 56SBbc12.211.52.7 × 1.5pF, pL, lEUGC 3653, MCG 14-4-22, CGCG 362-36, CGCG 363-20, IRAS 07006+8427
NGC 231407 10 31.8+75 19 40E313.212.21.1 × 0.8vF, S, RUGC 3677, MCG 13-6-3, CGCG 348-32
NGC 233607 27 03.6+80 10 40SBbc11.110.47.1 × 3.9pB, pL, R, 2 st 11 nrUGC 3809, MCG 13-6-6, CGCG 348-34, IRAS 07184+8016, CGCG 349-4, KCPG 132A
NGC 2336 A07 56 15.1+78 00 47Sc14.413.71.7 × 1.7pB, pL, R, 2 st 11 nrUGC 4066, MCG 13-6-12, CGCG 349-11
NGC 234707 16 04.0+64 42 41Sb13.212.51.8 × 1.3vF, S, R, lbMUGC 3759, MCG 11-9-39, CGCG 309-26, IRAS 07112+6447, KCPG 128B, near SAO 14129
NGC 236607 28 54.8+69 12 58IBm11.511.18.1 × 3vF, pL, mbM, vS * inv, curved tailsUGC 3851, MCG 12-7-40, DDO 42, IRAS 07233+6917, CGCG 330-38, MK 71, KCPG 133B
NGC 240307 36 50.6+65 36 06SBc8.98.523.4 × 11.8!! cB, eL, vmE, vgmbMNUGC 3918, MCG 11-10-7, CGCG 309-40, IRAS 07321+6543, KARA 197, CGCG 310-3
NGC 244107 51 54.5+73 00 55SBb13.012.22 × 1.8vF, pSUGC 4036, MCG 12-8-15, CGCG 331-17, IRAS 07460+7308
NGC 246007 56 52.8+60 20 58Sab12.711.82.5 × 1.9F, S, R, S * in centreUGC 4097, MCG 10-12-21, CGCG 287-10, IRAS 07525+6028
NGC 252308 15 00.0+73 34 44SBbc12.611.92.9 × 1.8pB, pL, lE, lbM, * nrUGC 4271, MCG 12-8-31, CGCG 331-32, Arp 9, IRAS 08092+7343
NGC 2523 A08 04 08.4+74 02 53SBc14.513.81 × 0.7pB, pL, lE, lbM, * nrUGC 4166, MCG 12-8-24, CGCG 331-26, KUG 0758+741
NGC 2523 B08 12 56.8+73 33 49Sb14.814.02 × 0.3pB, pL, lE, lbM, * nrUGC 4259, MCG 12-8-30, CGCG 331-30, IRAS 08072+7342
NGC 2523 C08 17 44.2+73 19 05E514.313.31.5 × 0.8pB, pL, lE, lbM, * nrUGC 4290, MCG 12-8-32, CGCG 331-33, NPM1G +73.0036
NGC 254408 21 40.3+73 59 18SBa13.812.91.1 × 0.8eeF, pS, R, sev B st aroundUGC 4327, MCG 12-8-34, MK 87, IRAS 08159+7409, KCPG 160A, KUG 0815+741, CGCG 331-36
NGC 255008 24 33.7+74 00 43Sb/P13.612.81 × 0.4eeF, pS, cEUGC 4359, MCG 12-8-37, CGCG 331-39, IRAS 08188+7410
NGC 2550 A08 28 39.1+73 44 53Sc13.412.71.6 × 1.4eeF, pS, cEUGC 4397, MCG 12-8-43, CGCG 331-43, KUG 0823+739, IRAS 08230+7354
NGC 255108 24 50.2+73 24 45Sa13.112.11.6 × 1vF, S, F * in centreUGC 4362, MCG 12-8-38, CGCG 331-40, ARAK 162
NGC 259108 37 25.5+78 01 32Sc12.912.23 × 0.6F, S, E, lbMUGC 4472, MCG 13-7-1, CGCG 349-29, CGCG 350-1, IRAS 08307+7811
NGC 263308 48 04.6+74 05 57SBb/P12.912.22.3 × 1.5F, S, lEUGC 4574, MCG 12-9-13, VV 519, IRAS 08425+7416, CGCG 331-63, CGCG 332-10, CGCG 350-5, Arp 80, KCPG 169
NGC 263408 48 25.5+73 58 02E112.912.01.7 × 1.6F, S, lEUGC 4581, MCG 12-9-15, CGCG 331-66, CGCG 332-13
NGC 2634 A08 48 38.1+73 56 19SBbc14.313.51.8 × 0.4F, S, lEUGC 4585, MCG 12-9-16, CGCG 331-68, CGCG 332-15, IRAS 08433+7406
NGC 263608 48 24.4+73 40 18E014.713.80.4 × 0.4vF, S, 2 st 11·12 fUGC 4583, CGCG 331-67, CGCG 332-14, NPM1G +73.0043
NGC 264608 50 21.8+73 27 46SB013.112.11.3 × 1.3vF, S, 2 F st 2'.5 sfIC 511, UGC 4604, MCG 12-9-19, CGCG 332-19, ARAK 180, CGCG 331-69
NGC 265508 55 37.7+78 13 25SB0-a11.010.14.9 × 4.1vB, cL, lE 90°, gsvmbMUGC 4637, MCG 13-7-10, CGCG 349-33, IRAS 08491+7824, CGCG 350-7, Arp 225
NGC 271509 08 05.9+78 05 09SBc11.811.24.8 × 1.6pB, L, EUGC 4759, MCG 13-7-15, CGCG 350-12, IRAS 09018+7817
NGC 273209 13 25.0+79 11 16S012.911.92.1 × 0.9pB, S, E 45°, * 13 nfUGC 4818, MCG 13-7-16, CGCG 350-13
NGC 274809 13 43.0+76 28 33Sbc12.411.73.1 × 1.1pB, pL, E, vglbMUGC 4825, MCG 13-7-19, CGCG 350-14, IRAS 09080+7640, PRC C-28
NGC 390111 42 49.2+77 22 22Sc14.413.71.8 × 0.8pF, pL, r, Place doubtfulUGC 6675, MCG 13-9-1, CGCG 351-68, CGCG 352-6, KARA 496
NGC 412712 08 25.8+76 48 16Sc13.412.72.5 × 1.2F, pL, vlE, glbMUGC 7122, MCG 13-9-12, CGCG 352-19, IRAS 12060+7705
NGC 529513 38 39.3+79 27 34E-S015.314.30.4 × 0.4vF, vS, RMCG 13-10-9, CGCG 353-23, NPM1G +79.0112
NGC 564014 20 40.7+80 07 25Sa15.614.70.9 × 0.4eF, S, lECGCG 353-35, NPM1G +80.0106
IC 33403 45 17.1+76 38 15I/P12.511.32.5 × 2.1pB, S, * 13 inv sfUGC 2824, MCG 13-3-7, CGCG 346-6
IC 34203 46 48.4+68 05 44SBc9.18.421.4 × 20.9pB, vS, * 12 close nUGC 2847, MCG 11-5-3, CGCG 305-2, IRAS 03419+6756
IC 35604 07 46.3+69 48 43Sb/P11.410.65.9 × 3.9pF, pL, bM, * 8.5 4' nUGC 2953, MCG 12-4-11, CGCG 327-15, Arp 213, IRAS 04025+6940
IC 38104 44 28.4+75 38 23SBbc13.112.32.4 × 1.3F, S, bM, * 12 npUGC 3130, MCG 13-4-7, CGCG 347-6, IRAS 04378+7532
IC 39104 57 22.1+78 11 23Sc/P13.012.71.1 × 1.1F, S, RUGC 3190, MCG 13-4-11, CGCG 347-9, IRAS 04497+7806, KARA 155, KUG 0449+781
IC 39604 57 58.8+68 19 23S?13.012.12.1 × 1.5F, S, R, bMN, F D * sfUGC 3203, MCG 11-7-2, CGCG 306-7, IRAS 04527+6814, CGCG 307-1, KCPG 104
IC 44006 19 13.0+80 04 06Sab14.113.31.6 × 0.9vF, SUGC 3427, MCG 13-5-21, CGCG 348-16, KCPG 109, IRAS 06102+8005
IC 44206 36 11.9+82 58 08E-S013.912.90.9 × 0.9F, S, R, mbMUGC 3470, MCG 14-4-3, CGCG 362-22, KCPG 113A, CGCG 363-5, NPM1G +83.0016
IC 44506 37 21.0+67 51 36S014.213.21.2 × 0.9eF, S, R, B * sfUGC 3497, MCG 11-9-1, CGCG 308-33, KCPG 114A
IC 44906 45 40.8+71 20 37E213.512.51.7 × 1.3pF, S, R, bM, bet 2 D stUGC 3515, MCG 12-7-14, CGCG 330-12
IC 45006 52 12.3+74 25 39S0-a15.013.90.8 × 0.5vF, SUGC 3547, MCG 12-7-18, MK 6, IRAS 06457+7429, KUG 0645+744, NPM1G +74.0026, CGCG 330-17
IC 45106 52 51.8+74 28 48Sb14.613.81.3 × 1.1vF, SUGC 3550, MCG 12-7-19, CGCG 330-18
IC 46707 30 17.8+79 52 21SBc13.212.63.1 × 1.2vF, pS, ssF of 2336UGC 3834, MCG 13-6-7, CGCG 348-35, IRAS 07218+7958, CGCG 349-5, KCPG 132B
IC 49908 45 17.3+85 44 26Sa13.412.52.1 × 1.1pF, S, mbM, * nfUGC 4463, MCG 14-4-54, CGCG 363-46, CGCG 364-5, NPM1G +85.0024, most northern IC
IC 51209 03 49.0+85 30 06Sc12.912.21.8 × 1.3F, S, R, gbMUGC 4646, MCG 14-5-2, CGCG 363-49, CGCG 364-8, IRAS 08508+8541
IC 52008 53 42.1+73 29 27SBab12.611.71.5 × 1.3pB, pL, bM, * nrUGC 4630, MCG 12-9-26, CGCG 331-73, IRAS 08483+7340, ARAK 183, CGCG 332-25
IC 52909 18 32.9+73 45 35Sc12.311.93.3 × 1.3pF, pL, EUGC 4888, MCG 12-9-35, CGCG 332-38, IRAS 09134+7358
IC 217407 09 05.0+75 21 13SBa14.313.50.9 × 0.7eF, S, bMUGC 3666, MCG 13-6-2, CGCG 348-30
IC 217907 15 32.3+64 55 34E113.512.41.1 × 1.1* 13 in vF, vS neb [? = III 746]UGC 3750, MCG 11-9-38A, CGCG 309-25, KCPG 128A
IC 218407 29 24.9+72 07 43Sbc13.913.10.8 × 0.7vF, S, stell, rUGC 3852, MCG 12-7-41, MK 8, IRAS 07236+7213, KCPG 135A, CGCG 330-39, 7ZW 156, VV 644
IC 220907 56 14.2+60 18 14SBb14.313.71.1 × 0.9vF, S, lbMUGC 4093, MCG 10-12-17, MK 13, IRAS 07519+6026, CGCG 286-78, CGCG 287-8, KUG 0751+604
IC 238908 47 58.3+73 32 19SBb14.013.41.4 × 0.3vF, S, lbMUGC 4576, MCG 12-9-11, CGCG 331-64, IRAS 08425+7343, CGCG 332-11, VV 798

«Strasbourg-ESO Catalogue of Galactic Planetary Nebulae» Acker et al., 1992 [141]
PNGRADecMain IDPKIRASDiscovererIdentitiesoDiam
["]
rDiam
["]
Dist
[kpc]
Rvel
[km/s]
ExpVel
[km/s]
C* NameC* MagC* SP Type
PN G123.6+34.512 33 07+82 33 50IC 3568123+34.112317+8250AITKEN 1900ARO 56, VV 63, VV' 111 10. 1.31 -41.1 ± 0.8 7.8 (O-III)AG +82 365, AG82 147, BD +83 357, GCRV 7565, HD 109540B: 13.73, V: 13.45O3(H)
PN G142.1+03.403 36 08+60 03 47K 3-9403319+5953KOHOUTEK 1972 7.1 10. 10. (O-III), 10. (N-II)
PN G143.6+23.806 29 35+71 04 04EGB 4ELLIS et al 1984 111. PG 0623+71B: 12.79, V: 12.77
PN G144.5+06.504 07 01+60 55 03NGC 1501144+06.104026+6047HERSCHEL 1787ARO 44, VV 16, VV' 22 52. 2.0 :+36.2 ± 1.4 37.0 (O-III)AG82 26, CSI +60 -04027, GCRV 2334, PLX 894U: 14.34, B: 15.17, V: 14.39WC 6-7,OVI, WC early
PN G146.7+07.604 25 51+60 07 13M 4-18146+07.104215+6000MINKOWSKI 1959ARO 213 4. 4. -17.0 ± 12.0< 7.5 (O-III), 17.0 (N-II)AG82 31B: 14.22, V: 13.96WC 11
PN G147.8+04.104 13 15+56 56 54M 2- 2147+04.104091+5649MINKOWSKI 1947ARO 211, VV 18, VV' 24 6.1 7. -7.0 ± 25.0 14.0 (O-III)
PN G149.0+04.404 20 45+56 18 13K 4-4704166+5611KOHOUTEK 1969 0. 0.25

Quellenangaben

7«Der grosse Kosmos-Himmelsführer» von Ian Ridpath und Wil Tirion; Kosmos Verlag; ISBN 3-440-05787-9
9«Drehbare Sternkarte SIRIUS» von H. Suter-Haug; Hallwag-Verlag, Bern
15«Hartung's Astronomical Objects for Southern Telescopes» by David Malin and David J. Frew; Melbourne University Press 1995; ISBN 0-522-84553-3
19«Prodromus Astronomiae» Johannes Hevelius, 1690; DOI:10.3931/e-rara-456
21«Taschenatlas der Sternbilder» von Josef Klepesta und Antonin Rükl; Verlag Werner Dausien; ISBN 3-7684-2384-0
133Deepsky Atlas of the Hawaiian Astronomical Society; hawastsoc.org/deepsky
141Strasbourg-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
150IAU: The Constellations, 11. Oktober 2020; iau.org/public/themes/constellations
154Yale Bright Star Catalog, 15. Oktober 2020; tdc-www.harvard.edu/catalogs/bsc5.html
277«Historische Deep-Sky Kataloge» von Dr. Wolfgang Steinicke; klima-luft.de/steinicke (2021-02-17)