Sternbild Taurus (Stier)

Eigenschaften
Das Sternbild Taurus liegt nordwestlich von Orion und ist durch die beiden großen lockeren Sternhaufen, den Hyaden und den Plejaden, leicht zu identifizieren. Die hellsten Sterne der Hyaden bilden ein auffälliges V am Himmel, das besonders markant erscheint, wenn das Sternbild untergeht und es direkt über dem westlichen Horizont steht. In den meisten Darstellungen wird jedoch nur der Kopf des Stieres, wie er drohend auf den Jäger Orion herabblickt, mit den Sternen assoziiert. Auffällig sind auch die beiden Hornsterne beta und zeta Tauri, wobei der nördlichere zwar nicht zum Sternbild Auriga, jedoch meist zu dessen fünfeckigen Alignement gezählt wird. Die Fläche, welche von der Sternbildgrenze gemäß IAU umschlossen wird, beträgt 797 Quadratgrad. Das Zentrum des Sternbilds kulminiert jeweils etwa am 30. November um Mitternacht. [9, 15]
Sterne mit Eigennamen:
- α Tau: Aldebaran, Cor Tauri, Parilicium
- β Tau: Alnath, El Nath, Nath
- γ Tau: Hyadum I
- δ1 Tau: Hyadum II
- ε Tau: Ain, Oculus Boreus
- η Tau: Alcyone
- 16 Tau: Celaeno, Celieno, Celeno, "Lost Pleiad"
- 17 Tau: Electra
- 19 Tau: Taygeta, Taygete
- 20 Tau: Maia
- 21 Tau: Asterope
- 22 Tau: Sterope Ii
- 23 Tau: Merope
- 27 Tau: Atlas
- 28 Tau: Pleione
Deep-Sky Objektbeschreibungen
Mythologie und Geschichte
Als eines der ältesten Sternbilder war Taurus schon in den ersten Hochkulturen bekannt. Man vermutet, dass das Sternbild um 5000 v. Chr. gebildet wurde. In der griechischen Mythologie gibt es vom Stier die schöne Geschichte zu erzählen, die sich ereignete, als Zeus (Jupiter) sich in die Tochter des Königs Agenor, der in Tyrus in Phönizien herrschte, verliebte. Zeus verwandelte sich damals in einen Stier, um die jungfräuliche Europa zu entführen:

Hermes (Merkur) verließ das nach Athene benannte Land, schwang seine Flügel und stieg himmelan. Zeus rief ihn beiseite und trug ihm auf - ohne ihm seine wahre Absicht mitzuteilen -, sofort nach Phönizien zu gehen und im Gebirge die jungen Stiere des Königs an die Küste zu treiben. Dort vergnügte sich für gewöhnlich des großen Königs hübsche Tochter zusammen mit anderen Mädchen aus Tyrus.
Zeus verwandelte sich in einen schneeweißen, kräftigen und schönen Stier mit Hörnern, durchsichtig wie Edelstein. Er mischte sich unter die Herde und näherte sich so der lieblichen Europa. Diese bewunderte den prächtigen und friedfertigen Stier. Doch wenn er auch sanftmütig erschien, scheute sie sich doch zuerst, ihn zu berühren, kam aber dann doch heran und hielt ihm Blumen an den weißen Mund. Da freute sich der verliebte Zeus, und während er auf die Erfüllung seines Verlangens hoffte, küsste er ihre Hände. Bald spielte er mit ihr und sprang auf dem grünen Rasen herum, bald streckte er die schneeweiße Flanke im gelblichen Sand aus. Allmählich schwand Europas Furcht. Nun liess sich der Stier von den Händen des Mädchens die Brust kraulen und um die Hörner frische Kränze schlingen.
Endlich wagte es die königliche Jungfrau sogar, ohne zu ahnen wer sie da tragen sollte, sich auf den Rücken des Stieres zu setzen. Da entfernte sich der Gott unmerklich vom Land und der trockenen Küste und setzte listig den Fuß in die äußersten Wellen, ging mehr und mehr hinein und trug durch die Weiten des Meeres seine Beute. Ängstlich blickte Europa auf die sich langsam entfernende Küste zurück, hielt sich mit der Rechten an des Stieres Mähne fest und mit der Linken ihr leichtes Gewand. Der Wind bauschte sich darin und spielte mit ihrem blonden, langen Haar. Die Furcht verlieh ihr neue Anmut. Oft zog sie ihre Mädchenfüße vom Meer in die Höhe und fürchtete die Berührung des hochspritzenden Wassers, oft tauchte der Gott mit Arglist den Rücken in die Wellen, damit sie sich umso enger an seinem Hals festhielt. Als sie das andere Ufer erreicht hatten, stand Zeus plötzlich ohne seine Hörner da, und er hatte sich vom Stier in den Gott zurückverwandelt. Sie stiegen auf zum Himmel und die Prinzessin wurde seine Geliebte. [20, 77]

Nach einer anderen Variante dieser Erzählung hatte sich Zeus nicht selbst in einen Stier verwandelt, sondern er hatte der jungfräulichen Europa einen echten Stier geschickt, um sie aus dem Kreis ihrer Gespielinnen zu entführen. Dieser Stier irrte dann herrenlos in Kreta herum.
Der kretischen Königin Pasiphae gefiel dieser schöne Stier so sehr, dass sie den bekannten Kunsthandwerker Daidalos beauftragte, eine hölzerne, lebensnah nachgeahmte Kuh zu bauen. Daidalos versah diese innen hohle Kuh mit einer Klappe am Rücken und überzog sie dann mit Kuhhaut. Die wollüstige Pasiphae schlüpfte in diese Kuh, um ihrem Verlangen zu frönen. Auf der Wiese in der Nähe von Gortys weidete der Bulle, kam schließlich heran, ließ sich von der Attrappe täuschen und besprang die vermeintliche Kuh.
Aus dieser Verbindung entspross der Minotaurus, ein grässliches Mischwesen. Bald hatten die Inseleinwohner beschlossen, diesen Schandfleck vor den Augen der Welt zu verbergen und versteckten den Minotaurus in einem verschlungenen Bau, in einem finsteren Gemäuer. Der Stier jedoch, der dieses Wesen zeugte, wurde von Poseidon, dem Gott des Meeres, zur Strafe mit Raserei geschlagen. Von einer Bestrafung der lüsternen Pasiphae weiß man nichts. Dieser Stier, der auf der Insel Kreta rasend und als schlimme Plage umherirrte, sollte nun von Herakles in seiner siebenten Aufgabe, die ihm Eurysteus auftrug, lebend eingefangen und nach Argus gebracht werden.
In Anlehnung an die erste Erzählung gibt es die Bezeichnung Portitor Europae (Fährmann der Europa) und Proditor Europae (Verräter der Europa). An die zweite Erzählung erinnert der Name Amasius Pasiphaes (Liebhaber der Pasiphae). Weitere Namen sind Bos (Stier), Princeps Armenti (Führer der Herde) und eigenartigerweise auch Bubulcus (Ackerknecht, Ochsenknecht), ein Name der eher dem Bootes zustünde. [20]
Kataloge
HR | B | F | DM | HD | SAO | FK5 | IR | M* | ADS | VarID | RA | Dec | vMag | spType | dMag | Sep ["] | Remarks |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
HR 1023 | BD+04 532 | 21018 | 111161 | 2509 | Var? | 03 23 39.1 | +04 52 55 | 6.38 | G5III | 3.2 | 0.9 | S:Weak G-band. | |||||
HR 1028 | BD+12 473 | 21051 | 93416 | 2241 | 03 24 10.1 | +12 37 46 | 6.04 | K0III-IV | |||||||||
HR 1030 | ο | 1 | BD+08 511 | 21120 | 111172 | 121 | I | 1134 | 03 24 48.8 | +09 01 44 | 3.60 | G6IIIFe-1 | SB:1654.9d, K 4.4k/s, V0 -20.1k/s, asini 96.7. Unresolved by speckle interferometry. | ||||
HR 1036 | BD+18 484 | 21335 | 93436 | 2242 | D | 03 27 03.2 | +18 45 23 | 6.57 | A3Vnp | 0.0 | 0.1 | D:7.2, 7.2, sep. 0.1" listed by D. W. Dunham. Probably not occultation double.,G:Hyades group.,S:Lambda Boo star, Mg 4481 wk. | |||||
HR 1038 | ξ | 2 | BD+09 439 | 21364 | 111195 | 123 | 03 27 10.2 | +09 43 58 | 3.74 | B9Vn | S:B8Vn+B8Vn+B7Vn.,SB:Triple Sp. system of 2 sharp-line stars revolving in 7.1466d; this pair revolves in 145.10d around broad-line B7 star. | ||||||
HR 1039 | BD+12 477 | 21379 | 93439 | 03 27 18.7 | +12 44 06 | 6.28 | A0V s | ||||||||||
HR 1061 | 4 | BD+10 452 | 21686 | 93463 | 03 30 24.5 | +11 20 11 | 5.14 | A0Vn | |||||||||
HR 1065 | BD+27 515 | 21743 | 75970 | 2582 A | 03 31 20.8 | +27 34 19 | 5.96 R | A2V | 0.4 | 11.4 | D:B CPM, A3V, vsini 100k/s, both components. | ||||||
HR 1066 | 5 | BD+12 486 | 21754 | 93469 | 125 | I | 03 30 52.4 | +12 56 12 | 4.11 | K0II-IIIFe-0.5 | 2.0 | 0.0 | SB:4.5, 6.5v, sep. 0.011", 960.0d, K 8.3k/s, V0 +14.2k/s, asini 100. Unresolved by speckle interferometry 1980.94 and,SB:1981.68. | ||||
HR 1067 | BD+05 502 | 21755 | 111230 | 2247 | 03 30 45.4 | +06 11 19 | 5.94 | G8III | |||||||||
HR 1079 | 6 | BD+08 528 | 21933 | 111246 | 03 32 36.0 | +09 22 25 | 5.77 | B9IV | |||||||||
HR 1085 | BD+17 575 | 22072 | 93494 | 03 34 08.3 | +17 49 58 | 6.17 | K1IVFe-1 | ||||||||||
HR 1086 | 7 | BD+23 473 | 22091 | 75999 | 2616 | 1192 | 03 34 26.6 | +24 27 52 | 5.92 | A3V+A3V | 0.2 | 0.7 | D:AB 6.6 A3V, 6.7 A3V, 568.22y, a = 0.650" or 600y, a = 0.719". Combined mag., colors. C, 9.9v at 22" physical.,DYN:0.005". | ||||
HR 1089 | BD+05 511 | 22211 | 111273 | 03 34 49.2 | +06 25 04 | 6.49 | G0 | ||||||||||
HR 1099 | BD+00 616 | 22468 | 111291 | 2644 | V711 Tau | 03 36 47.3 | +00 35 16 | 5.71 | G9V | 2.7 | 6.6 | D:5.88 dG9, 8.83, B-V +0.99, U-B +0.79, K6V, 2101y, a = 8.023". Close radio binary.,DYN:0.055".,SB:ADS 2644A, 2.8378d, K 50.2k/s, V0 -14.0k/s, msin3i 0.227, asini 1.96.,VAR:RS 5.70 - 5.81V, 2.83782d. Min. migrate in period 13y. Brightest of 25 RS CVn binaries known in 1976. Also var. radio,VAR:emission. Radio flare star with variable polarization. Amp. in red light (6600 A) 0.11 mag. Star spots inferred to,VAR:be about 1100d cooler than surrounding photosphere. | |||||
HR 1101 | 10 | BD-00 572 | 22484 | 111292 | 1101 | I | 03 36 52.4 | +00 24 06 | 4.28 | F9IV-V | 10.0 | 396.0 | D:CPM? Position angles disagree by about 40d. | ||||
HR 1102 | BD+14 586 | 22522 | 93524 | D | 03 37 47.8 | +15 25 51 | 6.39 | A5IV | 0.0 | 0.1 | |||||||
HR 1103 | BD+20 602 | 22615 | 76045 | 1213 | 03 39 00.1 | +20 54 57 | 6.50 | Am,A5-F0 | G:Mel 22 #5006; Pleiades group. | ||||||||
HR 1110 | BD+16 484 | 22695 | 93536 | 2257 | 2661 | 03 39 25.7 | +16 32 12 | 6.16 | K0III | 0.0 | 0.3 | D:ADS 2661A, occultation double?, 7.1, 7.1v, sep. 0.3". Component B, 11.8v at 36" optical. | |||||
HR 1115 | 12 | BD+02 581 | 22796 | 111334 | 2258 | 03 39 51.1 | +03 03 25 | 5.57 | gG6 | ||||||||
HR 1118 | 11 | BD+24 529 | 22805 | 76073 | 1103 | D | 03 40 46.3 | +25 19 46 | 6.11 | A2IV | 2.0 | 0.0 | G:Not a member of the Pleiades.,SB:20.4870d, K 34.2k/s, V0 -5.2k/s, asini 7.63; 6.3, 8.3v, sep. 0.0004". | ||||
HR 1119 | BD-01 519 | 22819 | 130645 | 03 39 59.5 | -01 07 14 | 6.12 | K1III-IV | ||||||||||
HR 1126 | 13 | BD+19 578 | 23016 | 93557 | 2263 | 03 42 18.9 | +19 42 01 | 5.69 | B9Vne | S:Shell star. H alpha emission. | |||||||
HR 1132 | 14 | BD+19 582 | 23183 | 93568 | 03 43 47.2 | +19 39 54 | 6.14 | G8III | G:61 Cyg group. | ||||||||
HR 1137 | BD+20 621 | 23258 | 76121 | 03 44 28.1 | +20 55 43 | 6.10 | A0V | ||||||||||
HR 1140 | 16 | BD+23 505 | 23288 | 76126 | D | 1262 | 03 44 48.2 | +24 17 22 | 5.46 | B7IV | 2.0 | 0.0 | D:Suspected occultation binary, sep. 0.0062". Unresolved by speckle interferometry 1981.69.,G:Pleiades cluster; Mel 22 #447.,N:Celaeno; Celieno; Celeno; "Lost Pleiad". | ||||
HR 1142 | 17 | BD+23 507 | 23302 | 76131 | 136 | D | 03 44 52.5 | +24 06 48 | 3.70 | B6III e | 2.0 | 0.0 | D:Sep. 0.062". Occultation of 1972 Mar. 19 indicated mag. diff 3.4, sep. 0.010".,G:Pleiades cluster; Mel 22 #468; in reflection nebula; Pleiades nebula. Member assoc. Tau R1 at 110 pc.,N:Electra.,SB:4.0, 6.0, sep. 0.002", 100.46d, K 26.0k/s, V0 -0.3k/s, asini 30.7. Unresolved by speckle interferometry. | ||||
HR 1144 | 18 | BD+24 546 | 23324 | 76137 | D | 03 45 09.7 | +24 50 21 | 5.64 | B8V | 0.0 | 0.1 | G:Pleiades cluster; Mel 22 #541; embedded in reflection nebulosity. | |||||
HR 1145 | 19 | BD+24 547 | 23338 | 76140 | W | 1264 | 03 45 12.5 | +24 28 02 | 4.30 | B6IV | 1.5 | 0.0 | D:Primary is SB, 4.6, 6.1v, sep. 0.012". Visual pair 4.4, 8.1v, sep. 69".,G:Pleiades cluster; Mel 22 #563; embedded in reflection nebulosity.,N:Taygeta; Taygete.,RV:vsini 135k/s.,SB:1313d, K 8.0k/s, V0 +5.9k/s, asini 144.0. Unresolved by speckle interferometry. | ||||
HR 1149 | 20 | BD+23 516 | 23408 | 76155 | D | 1279 | 03 45 49.6 | +24 22 04 | 3.87 | B8III v | 0.0 | 0.0 | C:Color excess E(B-V) = +0.02.,D:Sep. 0.003". Unresolved by speckle interferometry 1981.69. Duplicity questioned.,G:Pleiades cluster; Mel 22 #785; in reflection nebula. Pleiades nebula. Member assoc. Tau R1 at 110 pc.,N:Maia.,S:C1 neutral carbon continuum shows discontinuities in UV.,VAR:Probably cst. Var. helium lines. | ||||
HR 1151 | 21 | BD+24 553 | 23432 | 76159 | 1283 | 03 45 54.4 | +24 33 17 | 5.76 | B8V | G:Pleiades cluster; Mel 22 #817.,N:Asterope. Sterope I. | |||||||
HR 1152 | 22 | BD+24 556 | 23441 | 76164 | D | 03 46 02.9 | +24 31 41 | 6.43 | A0Vn | 0.0 | 0.1 | D:Suspected occultation double.,G:Pleiades cluster; Mel 22 #859.,N:Sterope II. | |||||
HR 1153 | 29 | BD+05 539 | 23466 | 111400 | 1104 | 2750 | 03 45 40.4 | +06 03 00 | 5.35 | B3V | 7.3 | 66.2 | D:B possibly optical.,G:Member of the local association (Pleiades group); Cas-Tau OB1.,SB:ADS 2750A; B3, A7, 2.4079d, K 23k/s, V0 +17k/s, asini 0.762. | ||||
HR 1156 | 23 | BD+23 522 | 23480 | 76172 | W | V971 Tau | 03 46 19.6 | +23 56 54 | 4.18 | B6IVe v | D:Suspected double probably single star.,G:Pleiades cluster; Mel 22 #980; in reflection nebula; Pleiades nebula; member assoc. Tau R1 at 110 pc.,N:Merope.,VAR:Variable hydrogen emission. | ||||||
HR 1159 | BD+06 583 | 23526 | 111407 | W | 03 46 09.5 | +06 48 11 | 5.91 | G9III | |||||||||
HR 1165 | η | 25 | BD+23 541 | 23630 | 76199 | 139 | I | W | 03 47 29.1 | +24 06 18 | 2.87 | B7IIIe | 1.6 | 0.0 | C:Color excess E(B-V) = +0.03.,D:Component A is occultation double, sep. 0.031". B, C, D, 8.1 A0V, 8.1 Am(A5/F0/F2) and 8.7v F2V at 117" to 190".,D:Possibly second occultation companion at 0.001", unresolved by speckle interferometry. vsini of B 155k/s. Numerous,D:photometric determinations yield 6.3 for B component. The HD gives 8.1 for 23629 and the IDS indicates 8.1. Burnham,,D:Double Stars, gave 7.0 vis.,G:Pleiades cluster; Mel 22 #1432; in reflection nebula; Pleiades nebula; member assoc. Tau R1 at 110 pc.,N:ALCYONE. The brightest of the Pleiades.,R:Angular diameter = 0.0016".,RV:Rotationally unstable Be shell star. | ||
HR 1172 | BD+22 563 | 23753 | 76215 | D | 1321 | 03 48 20.9 | +23 25 16 | 5.45 | B8V | 2.0 | 0.1 | G:Pleiades cluster; Mel 22 #1823. | |||||
HR 1174 | 30 | BD+10 486 | 23793 | 93611 | 2778 | 1327 | 03 48 16.3 | +11 08 36 | 5.07 | B3V+F5V | 4.4 | 9.2 | D:Binary.,G:Cas-Tau OB1.,M:Old disk population runaway star.,RV:Comp. B +17.2k/s; F5V or F3Vp. | ||||
HR 1178 | 27 | BD+23 557 | 23850 | 76228 | 142 | 2786 | 1345 | 03 49 09.7 | +24 03 12 | 3.63 | B8III | 1.5 | 0.0 | D:Component A SB, 4.1, 5.6, sep. 0.006" and 0.019". B, 6.8v at 0.4".,G:Pleiades cluster; Mel 22 #2168.,N:Atlas.,SB:ADS 2786A, 1254.68d, K 14.5k/s, V0 -0.4k/s, asini 248. Unresolved by speckle interferometry 1981.68. | |||
HR 1180 | 28 | BD+23 558 | 23862 | 76229 | BU Tau | 03 49 11.2 | +24 08 12 | 5.09 | B8Vpe v | G:Pleiades cluster; Mel 22 #2181.,N:Pleione.,S:Shell star.,SB:Suspected long period.,VAR:Gamma Cas 4.77 - 5.50V. Var. may be clue to shell episodes. Shell ejection 1936 led to decrease in light 1937-1958.,VAR:Variable hydrogen emission. Shell spectrum shows phase changes every 17 or 34 yrs. | |||||||
HR 1183 | BD+23 563 | 23923 | 76244 | 03 49 43.5 | +23 42 42 | 6.17 | B8V | G:Pleiades cluster; Mel 22 #2425. | |||||||||
HR 1185 | BD+21 535 | 23950 | 76250 | 03 49 55.0 | +22 14 40 | 6.07 | B8III | G:Mel 22 #5025; Pleiades.,S:Spectra show Hg, Mn, Cr. | |||||||||
HR 1188 | BD+25 624 | 23985 | 76256 | 2799 | 1366 | 03 50 18.9 | +25 34 46 | 5.26 | A2V+A5V | 0.4 | 0.7 | D:5.81 A3V, 6.21 A5V, 62.28y, a = 0.430". Resolved by speckle interferometry 1983.93, sep. 0.66". | |||||
HR 1193 | BD+21 539 | 24154 | 76275 | D | 03 51 36.6 | +22 01 54 | 6.83 R | K0III | D:Suspected occultation double. | ||||||||
HR 1194 | BD+12 516 | 24155 | 93637 | V766 Tau | 03 51 15.8 | +13 02 45 | 6.30 | B9pSi | M:Old disk population runaway star.,VAR:Amp. 0.06y?, 2.53d. | ||||||||
HR 1199 | 31 | BD+06 594 | 24263 | 111469 | 2275 | W | 03 52 00.2 | +06 32 05 | 5.67 | B5V | 0.1 | 0.6 | |||||
HR 1201 | BD+16 523 | 24357 | 93650 | 1106 | 03 53 10.0 | +17 19 37 | 5.97 | F4V | G:In Taurus cluster; Mel 25 #6; the Hyades. | ||||||||
HR 1218 | 32 | BD+22 605 | 24740 | 76339 | 2283 | 03 56 52.1 | +22 28 41 | 5.63 | F2IV | ||||||||
HR 1221 | 33 | BD+22 607 | 24769 | 76343 | D | V817 Tau | 03 57 03.8 | +23 10 32 | 6.06 | B9.5IV | 2.0 | 0.0 | G:Not a member of the Pleiades.,SB:1.5919d, K 56.9k/s, V0 +25.0k/s, asini 1.16, sep. 0.00006". Alternate orbit 2.975272d, K57.6k/s, V0 +14.2k/s,,SB:asini 2.36. | ||||
HR 1222 | BD+24 599 | 24802 | 76350 | 03 57 26.4 | +24 27 43 | 6.16 | K0 | ||||||||||
HR 1224 | BD+05 564 | 24817 | 111516 | 03 57 01.7 | +06 02 24 | 6.09 | A2Vn | ||||||||||
HR 1233 | BD+09 524 | 25102 | 93710 | 03 59 40.7 | +10 19 51 | 6.37 | F5V | G:In Taurus cluster; Mel 25 #8; the Hyades. | |||||||||
HR 1237 | BD+16 544 | 25175 | 93716 | 04 00 36.9 | +17 17 48 | 6.32 | A0V | ||||||||||
HR 1238 | BD+17 666 | 25202 | 93721 | 2288 | W | 04 00 48.8 | +18 11 38 | 5.89 | F4V | 3.3 | 164.2 | G:In Taurus cluster; Mel 25 #137; the Hyades. | |||||
HR 1239 | λ | 35 | BD+12 539 | 25204 | 93719 | 150 | I | Lam Tau | 04 00 40.8 | +12 29 25 | 3.47 | B3V+A4IV | DYN:0.0042".,SB:3.9540d, K 55.4k/s, V0 +15.2k/s, asini 2.99. RV also varies in 33.025d, triple system. Masses 6.8, 1.8 and about 1,SB:solar.,VAR:EA 3.3 - 3.80p, B3V+A, 3.952955d, i 86d. | ||||
HR 1243 | BD+09 528 | 25330 | 111566 | 2938 | 04 01 46.1 | +09 59 52 | 5.67 | B5V | 5.2 | 12.0 | D:Component B, F8V, optical. Third component mag. diff 6.13v, at 100". | ||||||
HR 1251 | ν | 38 | BD+05 581 | 25490 | 111579 | 151 | 04 03 09.4 | +05 59 21 | 3.91 | A1V | |||||||
HR 1252 | 36 | BD+23 609 | 25555 | 76425 | I | 2965 | 04 04 21.7 | +24 06 21 | 5.47 | G0III+A4V | 0.0 | 0.0 | D:A is occultation binary, sep. 0.033", unresolved by speckle interferometry 1981.68. Spectrum binary; vsini of,D:early-type component 160k/s. AB, mag. diff 6.5v, sep. 25.5".,S:Also classified G1III + B9V. | ||||
HR 1253 | 40 | BD+05 584 | 25558 | 111585 | 04 03 44.6 | +05 26 08 | 5.33 | B3V | G:In HII region; Cas-Tau OB1. | ||||||||
HR 1254 | BD+07 592 | 25570 | 111586 | 04 03 56.6 | +08 11 50 | 5.46 | F2V | G:In Taurus cluster; Mel 25 #160; the Hyades. | |||||||||
HR 1256 | 37 | BD+21 585 | 25604 | 76430 | 1112 | I | W | 04 04 41.7 | +22 04 55 | 4.36 | K0+III-IIIaFe-0.2 | 5.0 | 137.2 | G:Hyades? | |||
HR 1257 | BD+02 645 | 25621 | 111590 | 2292 | 04 04 09.9 | +02 49 37 | 5.36 | F6IV | G:Wolf 630 group. | ||||||||
HR 1262 | 39 | BD+21 587 | 25680 | 76438 | W | 1452 | 04 05 20.2 | +22 00 32 | 5.90 | G5V | 2.7 | 170.1 | G:Hyades? | ||||
HR 1268 | 41 | BD+27 633 | 25823 | 76455 | GS Tau | 04 06 36.4 | +27 36 00 | 5.20 | B9pSi v | G:Pleiades group.,S:Underabundance of magnesium and oxygen.,SB:7.227424d, K 16.6k/s, V0 +2.3k/s, asini 1.62. Periods of rotation and revolution same.,VAR:Alpha CV 5.15 - 5.22V, 7.227424d. Earlier period 11.94d still frequently quoted. Lines of SiII, SrII, possibly TiII,VAR:var. | |||||||
HR 1269 | ψ | 42 | BD+28 619 | 25867 | 76461 | 2295 | 04 07 00.5 | +29 00 05 | 5.23 | F1V | |||||||
HR 1279 | BD+14 657 | 26015 | 93775 | 2999 | 1466 | 04 07 42.0 | +15 09 46 | 6.01 | F3V | 3.2 | 3.8 | D:CPM. B is dG8.,G:In Taurus cluster; Mel 25 #11; the Hyades.,VAR:ADS 2999, B-A varies from 2.95 to 3.55V. Uncertain which component varies. Delta Sct? | |||||
HR 1280 | BD+16 560 | 26038 | 93777 | I | 3006 | 04 07 59.4 | +17 20 23 | 5.89 | K5IIIb | 0.0 | 0.1 | D:Primary of ADS 3006 is occultation binary, sep. 0.05". Visual companion, 9.3v at 4.4", CPM. | |||||
HR 1283 | ω1 | 43 | BD+19 672 | 26162 | 93785 | 1115 | 04 09 10.0 | +19 36 33 | 5.50 | K2III | |||||||
HR 1284 | BD+13 648 | 26171 | 93784 | 2298 | 04 09 01.6 | +13 23 54 | 5.95 | B9.5V | |||||||||
HR 1287 | 44 | BD+26 686 | 26322 | 76485 | 1116 | IM Tau | 04 10 49.9 | +26 28 51 | 5.41 | F2IV-V | VAR:Delta Sct 5.37 - 5.44V, 0.144923d. Possible other periods 0.126535 and 0.126569d. Light curve composite of 0.1449,VAR:and 0.1120d. Amp. B-V 0.035, amp. U-B 0.015. Variations in U-B opposite in phase from B-V. | ||||||
HR 1292 | 45 | BD+05 601 | 26462 | 111648 | 2301 | W | 04 11 20.3 | +05 31 23 | 5.72 | F4V | 4.1 | 124.1 | G:In Taurus cluster; Mel 25 #14; the Hyades. | ||||
HR 1295 | BD+16 569 | 26546 | 93810 | 04 12 31.4 | +17 16 39 | 6.09 | K0III | ||||||||||
HR 1297 | BD+22 649 | 26571 | 76505 | 04 12 51.2 | +22 24 49 | 6.12 | B9IIIp:Si: v | VAR:Spectrum var. | |||||||||
HR 1307 | BD+09 549 | 26676 | 93821 | 04 13 34.8 | +10 12 44 | 6.23 | B8Vn | G:In reflection nebula; member assoc. Tau R2 at 135 pc. | |||||||||
HR 1308 | BD+08 651 | 26677 | 111671 | 3063 | 04 13 31.3 | +08 53 26 | 6.51 | A2m | 6.3 | 54.3 | D:B, 13.6v at 8"; C, optical. | ||||||
HR 1309 | 46 | BD+07 617 | 26690 | 111672 | 3064 | 04 13 33.1 | +07 42 58 | 5.29 | F2V+F5V | 0.2 | 0.1 | D:6.0 F2V, 6.1 F3V, 7.18y, a = 0.135". Resolved by speckle interferometry 1983.93, sep. 0.09".,DYN:0.024". | |||||
HR 1310 | BD+12 564 | 26703 | 93823 | 04 13 49.9 | +12 45 12 | 6.25 | K0 | G:Probably Hyades group. | |||||||||
HR 1311 | 47 | BD+08 652 | 26722 | 111674 | I | 3072 | 04 13 56.4 | +09 15 49 | 4.84 | G5III+A7V? | 2.2 | 1.2 | D:AB binary; C, 12v at 32" optical.,DYN:0.003".,G:Hyades? | ||||
HR 1315 | BD+09 550 | 26793 | 111680 | 04 14 36.3 | +10 00 40 | 5.22 | B9Vn | ||||||||||
HR 1319 | 48 | BD+15 603 | 26911 | 93836 | W | 1537 | 04 15 46.3 | +15 24 02 | 6.32 | F5V | 4.7 | 151.4 | G:In Taurus cluster; Mel 25 #20; the Hyades. | ||||
HR 1320 | μ | 49 | BD+08 657 | 26912 | 111696 | 1118 | 04 15 32.1 | +08 53 32 | 4.29 | B3IV | G:Cas-Tau OB1; member of Pleiades group. | ||||||
HR 1321 | BD+05 613 | 26913 | 111695 | 3085 B | V891 Tau | 04 15 25.8 | +06 11 59 | 6.93 | G5IV | 0.6 | 64.7 | D:CPM with HR 1322.,VAR:BY, 6.92 - 7.00V. The fainter component of ADS 3085. Amp. 0.06V, 6.8d rotational period traced by large scale,VAR:star-spot activity. | |||||
HR 1322 | BD+05 614 | 26923 | 111698 | 3085 A | V774 Tau | 04 15 29.2 | +06 11 12 | 6.31 | G0IV | 0.6 | 64.7 | D:CPM with HR 1321.,VAR:6.28 - 6.37V. | |||||
HR 1329 | ω2 | 50 | BD+20 724 | 27045 | 76532 | D | Var? | 04 17 15.6 | +20 34 43 | 4.94 | A3m | 2.0 | 0.1 | D:Duplicity questioned.,SB:Over 5300d?, 5.0, 7.0v, sep. 0.05". Unresolved by speckle interferometry. | |||
HR 1331 | 51 | BD+21 618 | 27176 | 76541 | 2313 | W | 04 18 23.2 | +21 34 45 | 5.65 | F0V | 2.0 | 0.1 | D:Visual primary is speckle-interferometric double, sep. 0.076". Visual companion 10.7v at 166".,G:In Taurus cluster; Mel 25 #24; the Hyades.,SB:4035d, K 9.1k/s, V0 +38.3k/s, asini 475. Resolved by speckle interferometry 1977, sep. 0.08"; 1983.93, sep. 0.15". | ||||
HR 1334 | BD+09 558 | 27236 | 111729 | 04 18 24.5 | +09 29 12 | 6.54 | A4III | ||||||||||
HR 1339 | 53 | BD+20 733 | 27295 | 76548 | 04 19 26.1 | +21 08 32 | 5.35 | B9IV | D:CPM with HR 1341.,G:Member of Pleiades group.,S:Manganese star showing enhanced gallium, strontium, yttrium, zirconium. Manganese 120 times normal.,SB:4.452064d, K 9.6k/s, V0 +12.5k/s, asini 0.587. Shortest period for binary Mn star. Unresolved by speckle,SB:interferometry. | ||||||||
HR 1341 | 56 | BD+21 623 | 27309 | 76551 | V724 Tau | 04 19 36.7 | +21 46 25 | 5.38 | A0pSi | D:CPM with 1339.,G:Member of Pleiades group.,VAR:0.07V, 1.569d (light and spectrum). | |||||||
HR 1346 | γ | 54 | BD+15 612 | 27371 | 93868 | 159 | I | S | 1553 | 04 19 47.6 | +15 37 39 | 3.65 | K0-IIIabCN1 | G:In Taurus cluster; Mel 25 #28; the Hyades.,N:Hyadum I.,VAR:Amp. 0.1V. | |||
HR 1348 | φ | 52 | BD+27 655 | 27382 | 76558 | I | 3137 | 04 20 21.3 | +27 21 03 | 4.95 | K1III | 3.7 | 50.0 | D:Optical.,G:Hyades? | |||
HR 1349 | BD+09 562 | 27386 | 93866 | I | A | 04 19 37.5 | +10 07 17 | 6.31 | K0 | D:Astrometric binary unresolved by speckle interferometry. | |||||||
HR 1351 | 57 | BD+13 663 | 27397 | 93872 | W | V483 Tau | 04 19 57.7 | +14 02 07 | 5.59 | F0IV | 7.9 | 34.9 | D:Binary.,G:In Taurus cluster; Mel 25 #30; the Hyades.,VAR:Delta Sct 5.56 - 5.59V, 0.054d. | ||||
HR 1354 | BD+18 624 | 27429 | 93874 | 04 20 25.1 | +18 44 33 | 6.12 | F3:V | G:In Taurus cluster; Mel 25 #32; the Hyades. | |||||||||
HR 1356 | 58 | BD+14 682 | 27459 | 93876 | V696 Tau | 04 20 36.3 | +15 05 43 | 5.26 | F0V | G:In Taurus cluster; Mel 25 #33; the Hyades.,VAR:Delta Sct 5.20 - 5.26V, 0.036d or double. | |||||||
HR 1358 | BD+13 665 | 27483 | 93878 | 04 20 52.8 | +13 51 51 | 6.17 | F6V | G:In Taurus cluster; Mel 25 #34; the Hyades.,SB:3.0591d, K 71.0k/s, V0 +36.1k/s, msin3i 0.493, asini 2.99, i 51d? vsini both components 12k/s. | |||||||||
HR 1360 | BD+05 631 | 27497 | 111756 | 2320 | 04 20 41.2 | +06 07 51 | 5.77 | G8III-IV | |||||||||
HR 1361 | BD+08 672 | 27505 | 111759 | 04 20 49.0 | +09 13 32 | 6.53 | A4V | ||||||||||
HR 1368 | 60 | BD+13 668 | 27628 | 93892 | W | V775 Tau | 04 22 03.5 | +14 04 38 | 5.72 | A3m | 7.1 | 109.2 | G:In Taurus cluster; Mel 25 #38; the Hyades.,S:Also classified F2IIIbmvs.,SB:2.1433d, K 26.6k/s, V0 +41.7k/s, asini 0.783. | ||||
HR 1369 | χ | 59 | BD+25 707 | 27638 | 76573 | 3161 | 04 22 34.9 | +25 37 45 | 5.37 | B9V | 3.0 | 19.4 | D:CPM. Component A suspected occultation double; component B, G2V, strong lithium.,RV:ADS 3161B, +36.8k/s. | ||||
HR 1370 | BD+20 744 | 27639 | 76571 | I | 3158 | 04 22 22.8 | +20 49 17 | 5.91 | M0IIIab+A,F | 3.0 | 2.0 | DYN:0.003". | |||||
HR 1373 | δ1 | 61 | BD+17 712 | 27697 | 93897 | 162 | I | W | 1582 | 04 22 56.1 | +17 32 33 | 3.76 | K0-IIICN0.5 | 8.7 | 109.6 | G:In Taurus cluster; Mel 25 #41; the Hyades.,N:Hyadum II.,SB:529.8d, K 3.0k/s, V0 +39.5k/s, asini 19.8. D. W. Dunham indicates 3.9, 13.0v, sep. 0.04".,VAR:Amp. 0.1V. | |
HR 1375 | BD+20 751 | 27742 | 76585 | D | 04 23 32.4 | +20 58 56 | 5.99 | B8IV-V | 0.0 | 0.2 | |||||||
HR 1376 | 63 | BD+16 586 | 27749 | 93900 | Var? | 04 23 25.0 | +16 46 38 | 5.64 | A1m | 2.0 | 0.0 | G:In Taurus cluster; Mel 25 #45; the Hyades.,S:Ca and Sc underabundant and probably also K. Violet part of spectrum indicates luminosity III; G-band region, V. Also,S:classified F1IIImVs.,SB:5.9, 7.9, sep. 0.0006", 8.4178d, K 37.6k/s, V0 +35.0k/s, asini 4.33. | |||||
HR 1378 | 62 | BD+23 684 | 27778 | 76591 | 3179 A | 04 23 59.8 | +24 18 04 | 6.36 | B3V | 1.9 | 29.1 | D:AB CPM. B is A0. Component A suspected occultation double.,RV:ADS 3179B, +17.1k/s. | |||||
HR 1380 | δ2 | 64 | BD+17 714 | 27819 | 93907 | W | 04 24 05.8 | +17 26 38 | 4.80 | A7V | 8.5 | 143.0 | G:In Taurus cluster; Mel 25 #47; the Hyades. | ||||
HR 1381 | 66 | BD+09 570 | 27820 | 111791 | 3182 | 04 23 51.9 | +09 27 39 | 5.12 | A3V | 0.1 | 0.3 | D:5.8 A3V, 5.9 A4V, 51.6y, a = 0.18", or 55.40y, a = 0.20".,DYN:0.007".,G:UMa stream. | |||||
HR 1385 | BD+18 633 | 27901 | 93918 | 04 24 57.1 | +19 02 30 | 5.98 | F4V | G:In Taurus cluster; Mel 25 #53; the Hyades. | |||||||||
HR 1387 | κ1 | 65 | BD+21 642 | 27934 | 76601 | 3201 | 1593 | 04 25 22.1 | +22 17 38 | 4.22 | A7IV-V | 0.0 | 0.1 | D:Kappa1 Tau is occultation double. Together with Kappa2 = HR 1388 they form a multiple system of at least,D:6 components.,G:In Hyades cluster; Mel 25 #54.,VAR:Delta Sct? | |||
HR 1388 | κ2 | 67 | BD+21 643 | 27946 | 76602 | 3201 | 1594 | 04 25 25.0 | +22 11 59 | 5.28 | A7V | 0.0 | 0.1 | D:See HR 1387.,G:In Hyades cluster; Mel 25 #55.,VAR:Delta Sct, 5.26 - 5.29V. | |||
HR 1389 | δ3 | 68 | BD+17 719 | 27962 | 93923 | 3206 | V776 Tau | 04 25 29.4 | +17 55 41 | 4.29 | A2IV | 3.7 | 1.5 | D:AB binary; C, 11v at 77" CPM.,G:Hyades cluster; Mel 25 #56.,M:A blue straggler.,R:Diam. 2.1 solar.,SB:57.25d, K 68.8k/s, V0 +23.0k/s, asini 50.6.,VAR:Amp. 0.02U, 57.25d. Also magnetic field period. | |||
HR 1391 | 70 | BD+15 621 | 27991 | 93925 | W | 04 25 37.3 | +15 56 27 | 6.46 | F7V | 0.0 | 0.1 | D:AP 7.2 dF5, 7.2, 13.15y, a = 0.133"; occultation binary. Component B, 12.4v at 126". Speckle interferometric sep. of,D:AP 0.093" 1980.94; 0.094" 1983.93.,G:Open cluster Mel 25 #57; the Hyades. | |||||
HR 1392 | υ | 69 | BD+22 696 | 28024 | 76608 | 2326 | W | Ups Tau | 04 26 18.5 | +22 48 49 | 4.28 | A8Vn | 1.9 | 0.0 | D:The visual primary is SB, 4.6, 6.5v, sep. 0.020". Component B, 12.5v at 110".,G:In Hyades cluster; Mel 25 #60.,N:Some sources call this Upsilon1 and HR 1399 Upsilon2 Tau; other catalogues reverse these designations. The,N:superscripts now rarely used and Upsilon retained for 69 Tau. | ||
HR 1394 | 71 | BD+15 625 | 28052 | 93932 | W | V777 Tau | 04 26 20.8 | +15 37 06 | 4.49 | F0V | 2.0 | 0.1 | D:Visual primary is occultation double. Component B, 11.1 at 137".,G:In Taurus cluster; Mel 25 #141; the Hyades.,SB:5200d, K 15.1k/s, V0 +40.8k/s, asini 1050. Massive invisible component. Unresolved by speckle interferometry,SB:1983.93. | ||||
HR 1396 | π | 73 | BD+14 697 | 28100 | 93935 | I | 04 26 36.4 | +14 42 49 | 4.69 | G7IIIaFe-1 | |||||||
HR 1397 | BD+08 687 | 28114 | 111817 | 2327 | 04 26 21.1 | +08 35 25 | 6.06 | B6IV | |||||||||
HR 1399 | 72 | BD+22 699 | 28149 | 76613 | D | 04 27 17.5 | +22 59 47 | 5.53 | B7V | N:On nomenclature see HR 1392. | |||||||
HR 1400 | BD+01 753 | 28191 | 111827 | 04 27 00.7 | +02 04 46 | 6.23 | K1III | ||||||||||
HR 1402 | BD+10 577 | 28217 | 93943 | 3228 | 04 27 28.8 | +11 12 45 | 5.88 | B8IV | 1.8 | 0.4 | RV:Period possibly 19.83d or 20.43d. | ||||||
HR 1403 | BD+21 647 | 28226 | 76618 | W | 04 28 00.8 | +21 37 12 | 5.72 | Am | 0.8 | 0.0 | D:Primary is SB, 6.2, 7.0v, sep. 0.01". Visual secondary is 10.5v at 161", probably optical.,G:In Taurus cluster; Mel 25 #67; the Hyades. | ||||||
HR 1406 | BD+30 665 | 28271 | 57249 | 3243 A | 04 28 51.9 | +30 21 41 | 6.40 | F7V | 1.8 | 14.7 | D:AB binary; C, 11.32V at 121" optical. Fourth component 13.3v at 17" from C. | ||||||
HR 1407 | 75 | BD+16 605 | 28292 | 93950 | I | D | 1609 | 04 28 26.4 | +16 21 35 | 4.97 | K2III v | 2.5 | 0.0 | D:Sep. 0.024".,R:Diam. 0.0020". | |||
HR 1408 | 76 | BD+14 702 | 28294 | 93948 | 04 28 23.4 | +14 44 27 | 5.90 | F0IV | G:In Hyades cluster; Mel 25 #68. | ||||||||
HR 1409 | ε | 74 | BD+18 640 | 28305 | 93954 | 164 | I | W | 04 28 37.0 | +19 10 49 | 3.53 | G9.5IIICN0.5 | 7.0 | 181.6 | G:In Hyades cluster; Mel 25 #70.,N:Ain; Oculus Boreus. | ||
HR 1411 | θ1 | 77 | BD+15 631 | 28307 | 93955 | I | W | 04 28 34.5 | +15 57 44 | 3.84 | K0IIIbFe-0.5 | 0.4 | 337.4 | C:Color excess E(B-V) = +0.09.,D:CPM with HR 1412. Not clear if there are one or two occultation companions: mag. diff 3.8v, sep. 0.082", another,D:possible mag. diff 8v, sep. 0.2".,G:In Hyades cluster; Mel 25 #71.,R:Diam. 0.0026".,SB:6000 or 3000d. Unresolved by speckle interferometry 1983.93. | |||
HR 1412 | θ2 | 78 | BD+15 632 | 28319 | 93957 | W | The2 Tau | 04 28 39.7 | +15 52 15 | 3.40 | A7III | 0.4 | 337.4 | D:CPM with HR 1411. Close occultation binary, 3.5, 5.8v, sep. 0.005".,G:Member of Hyades cluster; Mel 25 #72.,SB:Sep. 0.005", 140.728d, K 31.0k/s, V0 +39.6k/s, asini 39.7, e 0.75.,VAR:Delta Sct, amp. 0.03V (variable), 0.080d. Possibly also eclipsing. | |||
HR 1413 | BD+01 755 | 28322 | 111840 | 04 28 03.6 | +01 51 31 | 6.15 | G9III | ||||||||||
HR 1414 | 79 | BD+12 598 | 28355 | 93960 | 2330 | 04 28 50.2 | +13 02 51 | 5.03 | A7V | G:Hyades cluster; Mel 25 #74. | |||||||
HR 1415 | BD+01 757 | 28375 | 111845 | 1123 | 04 28 32.1 | +01 22 51 | 5.55 | B3V | N:44 Eri in Tau. | ||||||||
HR 1420 | BD+10 583 | 28475 | 93968 | 04 29 42.9 | +10 31 18 | 6.79 | B5V | ||||||||||
HR 1422 | 80 | BD+15 636 | 28485 | 93970 | 3264 | 04 30 08.6 | +15 38 17 | 5.58 | F0V | 2.2 | 1.7 | D:5.7 F0V, 7.98 G2V, 189.5y, a = 1.01" (alternates 180.0y, a = 1.00"; 170y, a = 1.029"). Combined mass 2.82 solar.,D:Speckle interferometric sep. 1.300" (1980.94).,DYN:0.022".,G:In Hyades cluster; Mel 25 #80.,SB:ADS 3264A, 30.5d. | |||||
HR 1425 | BD+09 590 | 28505 | 93971 | 04 30 02.4 | +10 15 45 | 6.48 | G8III | ||||||||||
HR 1427 | BD+15 637 | 28527 | 93975 | W | 1627 | 04 30 33.7 | +16 11 38 | 4.78 | A6IV | 0.0 | 0.0 | D:Component A of visual pair is occultation double 5.6, 5.6v, sep. 0.02"; component B, 6.7v at 250".,G:In Hyades cluster; Mel 25 #82.,VAR:Delta Sct? | |||||
HR 1428 | 81 | BD+15 639 | 28546 | 93978 | W | 04 30 38.9 | +15 41 31 | 5.48 | A5m | 3.9 | 162.0 | G:In Hyades cluster; Mel 25 #83. | |||||
HR 1430 | 83 | BD+13 690 | 28556 | 93979 | W | 04 30 37.3 | +13 43 28 | 5.40 | F0V | 5.8 | 111.9 | G:In Hyades cluster; Mel 25 #84. | |||||
HR 1432 | 85 | BD+15 645 | 28677 | 93993 | 1640 | 04 31 51.8 | +15 51 06 | 6.02 | F4V | G:In Hyades cluster; Mel 25 #89. | |||||||
HR 1436 | BD+05 674 | 28736 | 111879 | 04 32 04.8 | +05 24 36 | 6.39 | F5V | G:In Hyades cluster; Mel 25 #90. | |||||||||
HR 1442 | BD+17 750 | 28867 | 94002 | 3297 | 04 33 32.9 | +18 01 00 | 6.25 | B9IVn | 0.1 | 3.1 | D:Binary. No change after 113y. | ||||||
HR 1444 | ρ | 86 | BD+14 720 | 28910 | 94007 | 1125 | Rho Tau | 04 33 50.9 | +14 50 40 | 4.65 | A8V | G:In Hyades cluster; Mel 25 #95.,SB:488.5d, K 18.5k/s, V0 +30.3k/s, asini 124. Unresolved by speckle interferometry. | |||||
HR 1445 | BD+28 666 | 28929 | 76654 | 3304 | 04 34 38.0 | +28 57 40 | 5.88 | B9pHg | 4.9 | 25.3 | S:Spectra show Hg; possibly Mn. | ||||||
HR 1446 | BD+09 600 | 28930 | 111890 | 04 33 48.1 | +09 24 47 | 6.01 | G8III | ||||||||||
HR 1448 | BD+05 679 | 28978 | 111896 | 2335 | 04 34 08.3 | +05 34 07 | 5.68 | A2V s | G:In Ursa cluster; UMa stream. | ||||||||
HR 1455 | BD+19 742 | 29104 | 94022 | 3316 | 04 35 42.7 | +19 52 54 | 6.36 | G5II-III+A-F | 0.5 | 0.3 | D:Visual duplicity questioned. Unresolved by speckle interferometry 1983.93. | ||||||
HR 1457 | α | 87 | BD+16 629 | 29139 | 94027 | 168 | I | 3321 | Alp Tau | 04 35 55.2 | +16 30 33 | 0.85 | K5+III v | 9.8 | 121.7 | D:AB binary. B is 13.5v, dM2 at 31". CD, 122" from A is 11.2, 13.6v sep. 2" also binary but independent of AB.,DYN:0.048".,G:Hyades group.,N:ALDEBARAN; Cor Tauri; Parilicium.,R:Diam. Two determinations, 0.022" and 0.0237".,S:IR emission envelope diam. 10". MgII emissions indicate a cooler shell surrounding the supergiant.,VAR:Lb 0.75 - 0.95V. Var. H and K emission. | |
HR 1458 | 88 | BD+09 607 | 29140 | 94026 | 3317 | 1658 | 04 35 39.3 | +10 09 39 | 4.25 | A5m | 3.6 | 69.7 | D:CPM. Companion 7.84V, +0.54(B-V), +0.04(U-B), F8V. vsini =<25k/s.,G:Hyades group.,R:Diam. relative to Sun = 2.2.,S:Also classified A6-7III-IVmw.,SB:ADS 3317A, 3.57124d, K 76.3k/s, V0 +28.7k/s, asini 3.75.,VAR:ADS 3317A, E?, 4.23 - 4.30V. | ||||
HR 1459 | BD+23 715 | 29169 | 76670 | 1663 | 04 36 29.2 | +23 20 27 | 6.02 | F5IV | G:In Taurus cluster; Mel 25 #100; the Hyades. | ||||||||
HR 1469 | BD+00 798 | 29335 | 111928 | 2339 | 1671 | 04 37 13.7 | +00 59 54 | 5.31 | B7V | N:49 Eri, in Tau.,VAR:5.3 - 5.38V. | |||||||
HR 1470 | BD+26 731 | 29364 | 76682 | 3353 | 1676 | 04 38 29.6 | +26 56 24 | 6.47 R | F2V: | 0.1 | 4.0 | D:Occultation indicated mag. diff 0.37v, sep. 2.117" (half the visual sep.) and PA 78d in contrast to visual 194d. | |||||
HR 1471 | BD+20 785 | 29365 | 76680 | 2341 | HU Tau | 04 38 15.8 | +20 41 05 | 5.92 | B8V | 1.5 | 0.0 | SB:6.0, 7.5v, sep. 0.0004", 2.0563d, K 65.4k/s, V0 -2.3k/s, asini 1.85. Masses 4 and 1.2 solar.,VAR:EA 5.92 - 6.7V, 2.056302d, period possibly variable. | |||||
HR 1472 | 89 | BD+15 661 | 29375 | 94043 | W | 04 38 09.4 | +16 02 00 | 5.79 | F0V | 5.9 | 140.5 | G:In Taurus cluster; Mel 25 #103; the Hyades. | |||||
HR 1473 | 90 | BD+12 618 | 29388 | 94044 | 2342 | W | 04 38 09.5 | +12 30 39 | 4.27 | A6V | 5.7 | 119.8 | G:In Taurus cluster; Mel 25 #104; the Hyades. | ||||
HR 1477 | BD+24 674 | 29459 | 76689 | 2343 | 04 39 23.1 | +25 13 06 | 6.22 | A5Vn | |||||||||
HR 1478 | σ1 | 91 | BD+15 665 | 29479 | 94051 | W | 04 39 09.2 | +15 47 59 | 5.07 | A4m | 0.4 | 431.2 | D:Binary with HR 1479 at 431" and with fainter SB companion, 7.4v at 0.0015".,G:Hyades?,SB:251.205d, K 5.0k/s, V0 +17.0k/s, asini 16.3. Unresolved by speckle interferometry. | ||||
HR 1479 | σ2 | 92 | BD+15 666 | 29488 | 94054 | 2345 | W | 04 39 16.5 | +15 55 05 | 4.69 | A5Vn | 0.4 | 431.2 | D:Binary with HR 1478.,G:Hyades cluster; Mel 25 #108. | |||
HR 1480 | BD+07 681 | 29499 | 111954 | 2344 | W | 04 39 06.2 | +07 52 15 | 5.39 | A5m | 3.5 | 297.8 | G:In Taurus cluster; Mel 25 #107; the Hyades. | |||||
HR 1484 | 93 | BD+11 639 | 29589 | 94063 | 04 40 03.4 | +12 11 52 | 5.46 | B8IV | S:Spectra show Hg, Mn. | ||||||||
HR 1490 | BD+28 680 | 29646 | 76707 | 1126 | 3379 | 04 41 19.8 | +28 36 54 | 5.78 | A2V | 5.2 | 43.5 | D:AB, CPM. Third component by Wallenquist, mag. diff 6.42, sep. 90". | |||||
HR 1497 | τ | 94 | BD+22 739 | 29763 | 76721 | 174 | W | 04 42 14.7 | +22 57 25 | 4.28 | B3V | 0.7 | 0.1 | D:AB CPM, 4.3, 8.9v sep. 0.1", 28y? C, 7.3A1V at 63" vsini 100k/s, physical. D. W. Dunham gives 4.9, 5.6v sep. 0.1" and,D:4.9, 6.4 sep. 0.0005".,G:Cas-Tau OB1.,SB:2.9565d, K 53.6k/s, V0 +12.3k/s, msin3i 2.96, asini 2.18. Resolved by speckle interferometry 1983.93,,SB:sep. 0.26". | |||
HR 1499 | 95 | BD+23 733 | 29859 | 76727 | 04 43 13.8 | +24 05 20 | 6.13 | F7IV-V | |||||||||
HR 1512 | BD+23 739 | 30122 | 76737 | 04 45 42.5 | +23 37 41 | 6.35 | B5III | G:Member of the local association (Pleiades group). | |||||||||
HR 1517 | BD+18 719 | 30197 | 94112 | 04 46 16.8 | +18 44 06 | 6.01 | K4III | G:Mel 25 #164; the Hyades, probable nonmember. | |||||||||
HR 1537 | 96 | BD+15 687 | 30605 | 94151 | I | 3464 | 04 49 44.1 | +15 54 15 | 6.08 | gK3 | 5.5 | 29.3 | |||||
HR 1547 | 97 | BD+18 743 | 30780 | 94164 | 1135 | W | V480 Tau | 04 51 22.5 | +18 50 23 | 5.10 | A7IV-V | 5.3 | 177.0 | G:In Hyades cluster; Mel 25 #123.,VAR:Delta Sct 5.09 - 5.11V, 0.042d. | |||
HR 1554 | BD+27 701 | 30912 | 76802 | 2365 | 04 52 47.1 | +27 53 51 | 5.97 | F2IV | G:Hyades moving group. | ||||||||
HR 1566 | BD+19 811 | 31236 | 94199 | 04 54 58.3 | +19 29 07 | 6.37 | F3IV | G:In Taurus cluster; Mel 25 #126; the Hyades. | |||||||||
HR 1575 | BD+24 709 | 31362 | 76848 | 04 56 15.6 | +24 35 32 | 6.37 | F0 | ||||||||||
HR 1585 | BD+16 672 | 31539 | 94227 | I | D | 04 57 22.3 | +17 09 13 | 5.48 | gK1 | 0.0 | 0.1 | R:Diam. 0.0017". | |||||
HR 1586 | 99 | BD+23 777 | 31553 | 76858 | 3557 | 04 57 48.7 | +23 56 55 | 5.79 | gG8 | 6.4 | 103.5 | ||||||
HR 1590 | 98 | BD+24 717 | 31592 | 76862 | 2374 | 3547 | 04 58 09.4 | +25 03 01 | 5.81 | A0V | 5.8 | 94.6 | D:Component A suspected occultation double. Two visual companions.,RV:Two determinations of vsini, 170 and 50k/s. | ||||
HR 1620 | ι | 102 | BD+21 751 | 32301 | 76920 | 184 | D | 05 03 05.7 | +21 35 24 | 4.64 | A7V | 0.0 | 0.1 | D:Probable double, 5.4, 5.4v, sep. 0.4".,G:Hyades cluster; Mel 25 #129. | |||
HR 1632 | BD+27 723 | 32480 | 76941 | 05 04 37.9 | +27 41 46 | 6.60 | F0III | ||||||||||
HR 1633 | BD+21 755 | 32482 | 76939 | 05 04 21.6 | +21 16 41 | 6.19 | K0 | ||||||||||
HR 1642 | BD+19 847 | 32642 | 94306 | 3672 | 05 05 32.1 | +19 48 23 | 6.44 | A5m | 0.6 | 1.1 | |||||||
HR 1656 | 104 | BD+18 779 | 32923 | 94332 | 3701 | 05 07 27.0 | +18 38 42 | 5.00 | G4V | 0.1 | 0.1 | D:5.6 G4V, 5.6 G4V, 1.19y, a = 0.18"; or 2.38y, a = 0.10"; or 5.8y, a = 0.11". Combined mag., colors. Sep. 0.099".,D:Unresolved by speckle interferometry 1983.93.,DYN:Uncertain, 0.023" to 0.138".,G:Hyades? | |||||
HR 1658 | 106 | BD+20 885 | 32977 | 76971 | 2383 | 05 07 48.4 | +20 25 06 | 5.30 | A5V | G:Hyades? | |||||||
HR 1659 | 103 | BD+24 755 | 32990 | 76974 | 3709 | 05 08 06.6 | +24 15 55 | 5.50 | B2V e | 5.7 | 35.3 | D:A is SB, 5.7, 7.7v sep. 0.0004". Visual companions 12.0 at 13", 8.6 at 35".,G:Cas-Tau OB1.,S:Shell star. H alpha double in emission.,SB:ADS 3709A, B0.5, B9.5, 58.31d, K 36.7k/s, V0 +16.2k/s, asini 28.9. | |||||
HR 1660 | 105 | BD+21 766 | 32991 | 76972 | W | 05 07 55.5 | +21 42 17 | 5.89 | B2Ve | 0.0 | 0.3 | D:Primary of visual pair is possible occultation double, 6.8, 6.8v, sep. 0.3"; secondary, 9.1v at 111.5" is BD +21d764.,G:Cas-Tau OB1.,RV:Pole on, but large range in RV in about 13y period.,S:Shell star. | |||||
HR 1670 | BD+27 732 | 33204 | 76990 | 1141 | 3730 A | 05 09 45.1 | +28 01 50 | 6.01 | A5m | 2.5 | 11.6 | D:BC 8.6 dG7, 9.1, 32.1y, a = 0.217". CPM with component A.,G:Hyades group and cluster; Mel 25 #131.,S:Also classified A9Vmvs. | |||||
HR 1711 | 108 | BD+22 864 | 34053 | 77057 | W | 05 15 27.7 | +22 17 05 | 6.27 | A2V | 6.2 | 1.9 | ||||||
HR 1739 | 109 | BD+21 816 | 34559 | 77097 | 2398 | I | 05 19 16.6 | +22 05 47 | 4.94 | G8III | |||||||
HR 1741 | BD+19 893 | 34579 | 77098 | 3894 | 05 19 14.7 | +20 08 05 | 6.08 | G8II-III+G1IV-V | 3.5 | 9.0 | D:CPM. Companion 9.64V, +0.76(B-V), +0.19(U-B), G1IV-V. | ||||||
HR 1750 | BD+27 758 | 34762 | 77121 | 05 20 59.3 | +27 57 26 | 6.33 | B9IV | 2.0 | 0.0 | SB:6.5, 8.5v, sep. 0.00002", 5.4337d, K 26.8k/s, V0 +5.8k/s, asini 2.00. | |||||||
HR 1755 | BD+19 902 | 34810 | 94478 | 05 20 56.6 | +19 48 51 | 6.18 | K0III | ||||||||||
HR 1774 | 110 | BD+16 765 | 35189 | 94514 | 05 23 37.7 | +16 41 58 | 6.08 | A2IV | |||||||||
HR 1780 | 111 | BD+17 920 | 35296 | 94526 | W | 05 24 25.4 | +17 23 00 | 4.99 | F8V | 2.9 | 85.7 | D:Companion optical. | |||||
HR 1791 | β | 112 | BD+28 795 | 35497 | 77168 | 202 | I | W | 05 26 17.5 | +28 36 27 | 1.65 | B7III | 33.4 | C:Color excess E(B-V) = 0.00.,G:Member of Pleiades group.,N:ALNATH; EL NATH; Nath. Beta Tau is also Gamma Aur, in Taurus.,RV:Expanding circumstellar shell.,S:Manganese star. | |||
HR 1798 | 113 | BD+16 775 | 35532 | 94543 | 05 26 05.7 | +16 42 01 | 6.25 | B2Vn | |||||||||
HR 1808 | 115 | BD+17 928 | 35671 | 94554 | 1148 | 4038 | 05 27 10.1 | +17 57 44 | 5.42 | B5V | 1.2 | 0.1 | D:ADS 4038A is occultation double. B and C are 10.1v at 305" and 11.8v at 343".,G:Member of the local association (Pleiades group); Cas-Tau OB1. | ||||
HR 1810 | 114 | BD+21 847 | 35708 | 77184 | 4048 | 05 27 38.1 | +21 56 13 | 4.88 | B2.5IV | 0.0 | 0.1 | D:ADS 4048A is occultation double, equal magnitudes, discovered during occultation of Feb. 26, 1901 by Innes. The three,D:visual companions: B, 12.39V at 38"; C, 11.55V at 59"; and D, 11.6 at 74" may all be CPM with A; however, B and C may,D:possibly be optical.,G:Cas-Tau OB1. | |||||
HR 1814 | 116 | BD+15 826 | 35770 | 94566 | 05 27 45.6 | +15 52 27 | 5.50 | B9.5Vn | |||||||||
HR 1816 | 117 | BD+17 931 | 35802 | 94573 | I | 05 28 01.6 | +17 14 20 | 5.77 | M1III | ||||||||
HR 1821 | 118 | BD+25 839 | 35943 | 77201 | 4068 A | 2009 | 05 29 16.5 | +25 09 02 | 5.47 | B8.5V | 0.8 | 4.8 | D:AB binary, B is A0V; colors for combined light. C, 11.5v at 141".,RV:ADS 4068B, +20k/s; vsini 197k/s. | ||||
HR 1831 | BD+22 925 | 36160 | 77220 | 05 30 43.4 | +22 27 45 | 6.29 | K0 | ||||||||||
HR 1845 | 119 | BD+18 875 | 36389 | 94628 | I | CE Tau | 05 32 12.8 | +18 35 40 | 4.38 | M2Iab-Ib e | C:Large infrared excess.,R:Diam. 0.0105".,S:Ultraviolet FeII emission.,VAR:SRc 6.1 - 6.5p, 165d. | ||||||
HR 1847 | BD+16 794 | 36408 | 94630 | 4131 A | 05 32 14.2 | +17 03 29 | 5.46 R | B7IIIe | 0.4 | 9.6 | D:Companion is B7IV, vsini 291k/s, optical.,SB:ADS 4131A. | ||||||
HR 1858 | 120 | BD+18 877 | 36576 | 94649 | V960 Tau | 05 33 31.6 | +18 32 25 | 5.69 | B2IV-Ve | RV:Pole on?,S:Shell star.,VAR:Gamma Cas, 5.53 - 5.69V. | |||||||
HR 1860 | BD+20 989 | 36589 | 77255 | 2132 | 05 33 38.8 | +20 28 27 | 6.18 | B6V | |||||||||
HR 1875 | 121 | BD+23 954 | 36819 | 77285 | 2415 | Var? | 05 35 27.1 | +24 02 22 | 5.38 | B2.5IV | G:Member of the local association (Pleiades group); Cas-Tau OB1.,SB:7.83552d. | ||||||
HR 1878 | BD+27 806 | 36859 | 77295 | I | 05 35 55.5 | +27 39 44 | 6.27 | K0 | |||||||||
HR 1889 | BD+25 879 | 36994 | 77310 | 05 36 30.2 | +25 56 22 | 6.49 | F5III | ||||||||||
HR 1902 | BD+26 870 | 37098 | 77322 | 4208 | 2426 | 05 37 08.8 | +26 55 27 | 5.83 | B9IV-V | 0.1 | 1.1 | D:AB binary, both components B8IV. Combined magnitude and colors. | |||||
HR 1905 | 122 | BD+16 822 | 37147 | 94700 | 05 37 03.8 | +17 02 25 | 5.54 | F0V | G:Mel 25 #168; Hyades cluster. | ||||||||
HR 1910 | ζ | 123 | BD+21 908 | 37202 | 77336 | 211 | I | D | Zet Tau | 05 37 38.7 | +21 08 33 | 3.00 | B4IIIpe v | 2.0 | 0.0 | C:Color excess E(B-V) = +0.09.,G:Cas-Tau OB1.,RV:Rapidly rotating star. Rotational velocity varies with wavelength: vsini about 300k/s in visual, 150 or less in UV.,RV:Expanding circumstellar shell. Shell-line velocities do not correspond to orbital elements; possibly gaseous ring.,RV:Unstable shell star with pseudo-periodic phenomena.,S:Lyman beta observed from COPERNICUS. Spectra obtained from AEROBEE rocket show absorption features at 1920 (FeIII),S:and 1720A (AlII) associated with extended atmosphere or circumstellar shell. Also classified B2IVp.,SB:132.91d, K 8.9k/s, V0 +21.8k/s, asini = 16.1. 3.2, 5.2v, sep. 0.007". Common circumstellar envelope. The 132.9d,SB:period is superimposed on a 7y pseudo-period related to oscillation of envelope.,VAR:Gamma Cas 2.90 - 3.03V. Var. shell Sp. Widths H-lines vary in about 10 min. Polarization at H beta changes in tens,VAR:of minutes, probably due to circumstellar matter. | |
HR 1921 | BD+26 884 | 37329 | 77350 | D | 05 38 57.4 | +26 37 04 | 6.37 R | G9III | D:Suspected occultation double. | ||||||||
HR 1928 | 125 | BD+25 902 | 37438 | 77360 | 2424 | D | 05 39 44.2 | +25 53 49 | 5.18 | B3IV | 2.0 | 0.0 | D:Triple system: SB and third component 8.5v at 0.32".,G:Cas-Tau OB1; member of Pleiades group.,SB:5.2, 7.2, sep. 0.0003", 27.864d, K 25.5k/s, V0 +14.8k/s, asini 8.16. | ||||
HR 1929 | BD+21 918 | 37439 | 77358 | 05 39 27.0 | +21 45 46 | 6.34 R | A1Vn | ||||||||||
HR 1946 | 126 | BD+16 841 | 37711 | 94759 | 4265 | 2560 | 05 41 17.7 | +16 32 02 | 4.86 | B3IV | 0.4 | 0.4 | D:5.3 B3IV, 5.9 B3V, 95.36y, a = 0.357". Equal components. Combined mag., colors.,DYN:0.004".,G:Member of the local association (Pleiades group); Cas-Tau OB1.,VAR:ADS 4265B, Beta C? 6.2 - 7.0v. | ||||
HR 1951 | BD+23 1007 | 37752 | 77413 | 05 41 54.6 | +23 19 35 | 6.59 | B8p | S:Possibly Hg in spectrum. | |||||||||
HR 1954 | BD+22 996 | 37784 | 77420 | 05 42 03.9 | +22 39 37 | 6.36 R | K2 | ||||||||||
HR 1961 | BD+23 1015 | 37967 | 77450 | V731 Tau | 05 43 19.5 | +23 12 15 | 6.21 | B2.5Ve | G:Cas-Tau OB1.,VAR:Amp. about 0.04V. | ||||||||
HR 1977 | BD+20 1083 | 38307 | 77516 | I | Y Tau | 05 45 39.4 | +20 41 42 | 6.95 | C5II | R:Occultation diam. = 0.0080 - 0.0088".,RV:Sign uncertain.,VAR:SRa 10.1 - 12.2p, 240.9d. Mean mag. varies in period 1750d. | |||||||
HR 1985 | 129 | BD+15 926 | 38478 | 94848 | 05 46 45.5 | +15 49 21 | 6.00 | B8IIIpHgMn: | |||||||||
HR 1989 | 131 | BD+14 1025 | 38545 | 94855 | 05 47 13.2 | +14 29 18 | 5.72 | A3Vn | |||||||||
HR 1990 | 130 | BD+17 1004 | 38558 | 94858 | 218 | 05 47 26.2 | +17 43 45 | 5.49 | F0III | ||||||||
HR 1993 | 133 | BD+13 979 | 38622 | 94864 | 2433 | 4381 | 05 47 42.9 | +13 53 59 | 5.29 | B2IV-V | 6.1 | 24.9 | D:Component B optical.,G:Member of the local association (Pleiades group); Cas-Tau OB1. | ||||
HR 1997 | BD+20 1105 | 38670 | 77578 | 4392 | 05 48 22.4 | +20 52 10 | 6.07 | B9Vn | 1.4 | 0.5 | D:AB binary. C, 7.2v A0 at 75", CPM.,SB:ADS 4392A. | ||||||
HR 2002 | 132 | BD+24 970 | 38751 | 77592 | 2435 | I | D | 2650 | 05 49 01.0 | +24 34 03 | 4.86 | G8III v | 0.0 | 0.1 | |||
HR 2010 | 134 | BD+12 912 | 38899 | 94888 | W | 05 49 32.9 | +12 39 04 | 4.91 | B9IV | 5.4 | 18.9 | ||||||
HR 2013 | BD+27 888 | 39004 | 77625 | 4474 | 05 50 58.1 | +27 58 04 | 5.56 | gG7 | 1.3 | 0.0 | D:Third component, visual, 11.6v at 15". Reality of the occultation binary, sep. 0.01", has been questioned.,R:Occultation diam. = 0.0024". | ||||||
HR 2016 | 135 | BD+14 1041 | 39019 | 94904 | 05 50 28.9 | +14 18 20 | 5.52 | gG9 | |||||||||
HR 2033 | 137 | BD+14 1060 | 39317 | 94945 | V809 Tau | 05 52 22.3 | +14 10 18 | 5.59 | B9pSiCrEu | VAR:Amp. 0.05U, 2.63?d. Possible new periods of 2.654 and 1.5889d, of which the smaller preferred. | |||||||
HR 2034 | 136 | BD+27 899 | 39357 | 77675 | 1158 | D | 2696 | 05 53 19.6 | +27 36 44 | 4.58 | A0V | 1.5 | 0.0 | SB:4.8, 6.3v, sep. 0.0013", 5.969d, K 48.9k/s, V0 -17.2k/s, msin3i 0.633, asini 4.01. | |||
HR 2074 | BD+24 1033 | 39970 | 77750 | 05 56 56.1 | +24 14 59 | 6.02 | A0Ia | G:Gem OB1. | |||||||||
HR 2084 | 139 | BD+25 1052 | 40111 | 77775 | 05 57 59.7 | +25 57 14 | 4.82 | B0.5II | C:Color excess E(B-V) = +0.15.,G:Gem OB1.,S:uv indicates gB0.5. |
Planetarische Nebel | ||||||||
---|---|---|---|---|---|---|---|---|
Name | RA | Dec | Typ | bMag | vMag | Dim | Dreyer Beschreibung | Identifikation, Anmerkungen |
NGC 1514 | 04 09 17.0 | +30 46 35 | PN | 10.0 | 10.9 | 2.2 | * 9m in neb 3' diam | PK 165-15.1, CS=9.4 |
Galaktische Nebel | ||||||||
Name | RA | Dec | Typ | bMag | vMag | Dim | Dreyer Beschreibung | Identifikation, Anmerkungen |
NGC 1432 | 03 45 49.5 | +24 22 06 | RN | 26 × 26 | eF, vL, dif (Maja Plejadum) | LBN 772, Maia nebula | ||
NGC 1435 | 03 46 10.0 | +23 45 54 | RN | 30 × 30 | vF, vL, dif (Merope) | CED 19I, Merope nebula | ||
NGC 1555 | 04 21 56.7 | +19 32 04 | RN | 0.5 | !!! vF, S, variable (Auw 20) | DG 31, CED 32B, vdB 28, Hind's variable nebula | ||
NGC 1952 | 05 34 31.9 | +22 00 52 | SNR | 8.4 | 6 × 4 | vB, vL, E 135° ±, vglbM, r | M 1, LBN 833, Sh2-244, CED 53, Taurus A, Crab nebula | |
IC 336 | 03 37 00.0 | +23 24 00 | EN | vF, eeL, v dif | ||||
IC 341 | 03 40 00.0 | +22 00 00 | EN | 135 | vF, eeL, v dif | CED 19B | ||
IC 349 | 03 46 20.0 | +23 56 23 | RN | 0.5 × 0.5 | eF, vS, Pos. 165°, Dist. 36" from Merope | CED 19I, Barnard's Merope nebula | ||
IC 353 | 03 53 00.3 | +25 48 00 | EN | 180 × 30 | vF, eeL, v dif | LBN 601, Ced 24 | ||
IC 354 | 03 53 00.0 | +23 00 00 | EN | 130 | vF, eeL, v dif | CED 19q | ||
IC 360 | 04 09 00.0 | +26 06 00 | EN | 180 × 100 | vF, eeL, v dif | LBN 786 | ||
IC 1990 | 03 47 13.8 | +24 20 02 | EN | vL, mE pf, 15' l | CED 19M | |||
IC 1995 | 03 50 18.5 | +25 34 51 | RN | 135 × 135 | * 6 in eF, eeL neb (M.N., lx. P. 260) | CED 22, Pos of SAO 76256 | ||
IC 2087 | 04 40 00.0 | +25 44 32 | RN | 4 × 4 | eeF, in hole of eL neby | LBN 813, CED 38 | ||
IC 2088 | 04 31 00.0 | +26 36 00 | EN | 360 | eeL, 3° long | LBN 793 | ||
IC 2144 | 05 50 14.0 | +23 52 20 | EN | 1 | pF, eS, * 12 nnp 2', * 12 s 1' | BFS 50 | ||
Offene Sternhaufen | ||||||||
Name | RA | Dec | Typ | bMag | vMag | Dim | Dreyer Beschreibung | Identifikation, Anmerkungen |
NGC 1647 | 04 45 42.2 | +19 07 09 | II2m | 6.4 | 40 | Cl, vL, st L, sc | OCL 457 | |
NGC 1750 | 05 03 54.0 | +23 39 30 | OCL | 25 × 12 | Cl, st L, vc sc | OCL 454 | ||
NGC 1758 | 05 04 36.0 | +23 47 54 | IV1p | 40 | Cl, pC, st L and S | OCL 453 | ||
NGC 1802 | 05 10 14.0 | +24 07 30 | OCL | 20 | Cl, st c sc | *Grp ? | ||
NGC 1807 | 05 10 46.0 | +16 30 48 | II2p | 7.0 | 12 | Cl, pRi, st L & S | OCL 462, * group? | |
NGC 1817 | 05 12 27.0 | +16 41 00 | III1m | 7.7 | 20 | Cl, L, Ri, lC, st 11…14 | OCL 463 | |
NGC 2026 | 05 43 12.0 | +20 08 00 | OCL | 10 | Cl, lRi, lC, st pL | |||
Galaxien | ||||||||
Name | RA | Dec | Typ | bMag | vMag | Dim | Dreyer Beschreibung | Identifikation, Anmerkungen |
NGC 1349 | 03 31 27.4 | +04 22 53 | S0 | 14.2 | 13.1 | 0.8 × 0.8 | eeF, S, R, bet 2 st | UGC 2774, MCG 1-9-6, CGCG 416-13, KARA 128, NPM1G +04.0118 |
NGC 1384 | 03 39 13.5 | +15 49 10 | Sc | 15.2 | 14.5 | 0.9 × 0.5 | Neb * 13 | MCG 3-10-3, CGCG 465-4 |
NGC 1409 | 03 41 10.4 | -01 18 07 | SB0 | 14.8 | 13.8 | 1 × 0.8 | eF, stellar or lE | UGC 2821, MCG 0-10-11, CGCG 391-28, KCPG 93A, VV 729, 3ZW 55, NPM1G -01.0133 |
NGC 1410 | 03 41 10.8 | -01 17 55 | E1 | 15.0 | 14.0 | 0.7 × 0.6 | Makes D neb with h 304, pos 0° | UGC 2821, MCG 0-10-12, CGCG 391-28, KCPG 93B, VV 729, 3ZW 55 |
NGC 1431 | 03 44 40.7 | +02 50 08 | S0 | 15.1 | 14.1 | 1 × 0.8 | eF, pL, iR | UGC 2845, MCG 0-10-17, CGCG 391-33, NPM1G +02.0129 |
NGC 1462 | 03 50 23.4 | +06 58 23 | S | 15.2 | 14.4 | 0.9 × 0.5 | vF, S, vlE | MCG 1-10-10, CGCG 417-7 |
NGC 1474 | 03 54 30.3 | +10 42 25 | SBa | 14.7 | 13.8 | 1.1 × 1 | vF, S, R | IC 2002, UGC 2898, MCG 2-10-3, CGCG 442-5, KARA 135 |
NGC 1497 | 04 02 06.8 | +23 08 00 | S0 | 14.1 | 13.1 | 1.5 × 0.7 | eF, vS, iR, mbM | UGC 2929, MCG 4-10-8, CGCG 487-9, NPM1G +22.0134 |
NGC 1508 | 04 05 47.6 | +25 24 33 | Sc | 15.2 | 14.5 | 0.7 × 0.6 | vF, vS, R, bM, r | MCG 4-10-21, CGCG 487-21, NPM1G +25.0119 |
NGC 1517 | 04 09 11.9 | +08 38 56 | Sc | 14.1 | 13.4 | 1.1 × 1 | vF, vS, R, r, * 9, 10 sf | UGC 2970, CGCG 418-13, IRAS 04064+0831 |
NGC 1539 1 | 04 19 01.9 | +26 49 39 | C | 15.8 | 14.8 | 0.5 × 0.5 | vF, vS, gbM | CGCG 488-1, 5ZW 373 |
NGC 1539 2 | 04 19 02.7 | +26 49 46 | C | 17.6 | 16.6 | 0.3 × 0.3 | vF, vS, gbM | CGCG 488-1, 5ZW 373 |
NGC 1541 | 04 17 00.2 | +00 50 07 | S0-a | 14.6 | 13.6 | 1.3 × 0.5 | vF, S | UGC 3001, MCG 0-11-40, CGCG 392-13 |
NGC 1542 | 04 17 14.1 | +04 46 55 | Sab | 14.7 | 13.9 | 1.3 × 0.5 | vF, S, E | UGC 3003, MCG 1-11-16, CGCG 418-17, KARA 145, IRAS 04145+0439 |
NGC 1551 | 04 19 38.1 | +02 24 34 | E-S0 | 13.1 | 12.0 | 2.2 × 1.9 | F, vS, R, probably = 835 | NGC 1550, UGC 3012, MCG 0-11-55, CGCG 393-1 |
NGC 1587 | 04 30 40.0 | +00 39 45 | E2 | 12.7 | 11.7 | 1.7 × 1.4 | F, pS, R, r, p of D neb | UGC 3063, MCG 0-12-35, CGCG 393-28, KCPG 99A, 2ZW 12 |
NGC 1588 | 04 30 43.7 | +00 39 55 | E5 | 13.9 | 12.9 | 1.1 × 0.6 | F, vS, R, r, f of D neb | UGC 3064, MCG 0-12-37, CGCG 393-29, KCPG 99B, MK 616, 2ZW 12, NPM1G +00.0155 |
NGC 1589 | 04 30 45.4 | +00 51 48 | Sab | 12.8 | 11.8 | 3.2 × 1 | F, pL, lE 132°, * 42°, 80" | UGC 3065, MCG 0-12-38, CGCG 393-30 |
NGC 1590 | 04 31 10.2 | +07 37 51 | S/P | 14.5 | 13.7 | 0.9 × 0.7 | F, S, * 12 nf | UGC 3071, MCG 1-12-8, CGCG 419-14, IRAS 04284+0731, 2ZW 13, KUG 0428+075 |
NGC 1593 | 04 32 06.1 | +00 34 04 | S0 | 14.4 | 13.4 | 1.6 × 0.6 | vF | NGC 1608, IC 2077, UGC 3082, MCG 0-12-44, CGCG 393-37, NPM1G +00.0156 |
NGC 1615 | 04 36 01.9 | +19 57 03 | E-S0 | 14.6 | 13.9 | 1.2 × 0.8 | vF, vS, R, lbM, vS * inv | UGC 3096, MCG 3-12-5, CGCG 467-3 |
NGC 1633 | 04 40 09.1 | +07 20 59 | SBab | 14.3 | 13.5 | 1 × 0.9 | eF, S, R, * 8 sp, p of D neb | UGC 3125, MCG 1-12-14, CGCG 419-23, KCPG 101A |
NGC 1634 | 04 40 09.8 | +07 20 20 | E-S0 | 15.1 | 14.1 | 0.4 × 0.3 | eF, vS, f of D neb | MCG 1-12-15, CGCG 419-22, ARAK 109, KCPG 101B |
NGC 1642 | 04 42 54.9 | +00 37 08 | Sc | 13.3 | 12.6 | 1.7 × 1.2 | F, R, Cometary, Δ with 2 st 18, f | UGC 3140, MCG 0-12-72, CGCG 393-73, IRAS 04403+0031 |
IC 322 | 03 26 00.5 | +03 40 49 | D | 15.2 | 14.6 | 0.9 × 0.8 | vF, pL, vlbM, diffic | CGCG 390-89, CGCG 416-8 |
IC 329 | 03 32 01.3 | +00 16 48 | S? | 15.2 | 14.3 | 0.9 × 0.4 | F, vS, R, lbM | MCG 0-10-1, CGCG 391-2, NPM1G +00.0135 |
IC 330 | 03 32 07.9 | +00 21 12 | Sab | 14.9 | 14.1 | 1.2 × 0.3 | F, vS, R, lbM | UGC 2779, MCG 0-10-2, CGCG 391-4 |
IC 331 | 03 32 19.0 | +00 16 58 | S | 14.7 | 13.9 | 0.9 × 0.9 | * 13 in neb | MCG 0-10-3, CGCG 391-5, IRAS 03296+0005 |
IC 332 | 03 32 37.4 | +01 22 59 | S0-a | 14.6 | 13.7 | 0.9 × 0.5 | F, vS, R, sbM | MCG 0-10-4, CGCG 391-6, KARA 129, NPM1G +01.0123 |
IC 338 | 03 37 38.1 | +03 07 06 | S? | 14.7 | 13.8 | 0.8 × 0.7 | vF, S, dif, vF * close | MCG 0-10-7, CGCG 391-18 |
IC 355 | 03 53 46.3 | +19 58 27 | Sc | 15.6 | 14.9 | 0.5 × 0.5 | vF, S, R, dif | MCG 3-10-10, CGCG 465-10, IRAS 03509+1949 |
IC 357 | 04 03 43.9 | +22 09 35 | SBab | 14.0 | 13.2 | 1.2 × 1 | F, S, R, N = 13.5 | UGC 2941, MCG 4-10-16, CGCG 487-16, NPM1G +22.0137, IRAS 04007+2201 |
IC 358 | 04 03 42.8 | +19 53 44 | S0 | 15.1 | 14.1 | 1 × 0.4 | vS, dif, lbM | UGC 2940, MCG 3-11-6, CGCG 466-9, NPM1G +19.0125 |
IC 359 | 04 12 28.4 | +27 42 11 | E-S0 | 14.9 | 13.9 | 1.3 × 1.3 | eeF, pL, R | UGC 2980, MCG 5-10-9, CGCG 508-8 |
IC 363 | 04 18 55.2 | +03 01 56 | C | 15.4 | 14.4 | 0.2 × 0.2 | eF, * 9 nf 3' | CGCG 392-19 |
IC 364 | 04 19 06.6 | +03 11 22 | E5 | 14.8 | 13.8 | 0.4 × 0.2 | vF, vS, R, sbM | CGCG 392-20, NPM1G +03.0150 |
IC 365 | 04 19 14.2 | +03 20 56 | S0-a | 14.8 | 13.9 | 1 × 0.6 | pB, S, iF, sbM | MCG 1-11-17, CGCG 392-21, IRAS 04166+0313 |
IC 366 | 04 19 41.5 | +02 21 37 | E3 | 15.7 | 14.7 | 0.3 × 0.2 | eF, 3' sf of 1550 | CGCG 393-2, NPM1G +02.0138 |
IC 374 | 04 32 32.8 | +16 38 06 | S | 15.7 | 14.9 | 0.8 × 0.4 | F, S, R, mbM | MCG 3-12-1, CGCG 467-1, ARAK 107 |
IC 383 | 04 38 58.0 | +09 53 33 | E0 | 15.8 | 14.8 | 0.4 × 0.4 | vF, S, dif, * 11.5 f | |
IC 1918 | 03 26 17.8 | +04 32 30 | S | 14.9 | 14.1 | 0.4 × 0.2 | F, S, glbM, dif | CGCG 416-9, NPM1G +04.0115 |
IC 1930 | 03 28 46.1 | +04 23 02 | E3 | 16.0 | 15.0 | 0.4 × 0.3 | F, S, R, gbM, * 8 p 3s, s 1'.6 | |
IC 1931 | 03 28 57.8 | +01 45 02 | D | 15.3 | 14.7 | 0.8 × 0.8 | vF, dif | MCG 0-9-87, CGCG 390-94 |
IC 1956 | 03 35 33.2 | +05 04 02 | SBbc | 15.4 | 14.6 | 1.6 × 0.3 | F, S, E 200°, 2 vF Nuclei | UGC 2795, MCG 1-10-1, CGCG 417-1, KARA 130, IRAS 03329+0454 |
IC 1967 | 03 37 47.8 | +03 16 13 | S? | 15.8 | 15.0 | 0.9 × 0.4 | vF, S, R, * 13 nr | MCG 0-10-8, CGCG 391-20, IRAS 03351+0306 |
IC 1977 | 03 40 45.0 | +17 44 27 | SBb | 14.3 | 13.5 | 1.4 × 0.8 | F, S, R, dif, * 13.5 nr | UGC 2815, MCG 3-10-5, CGCG 465-7, IRAS 03378+1734 |
IC 1998 | 03 51 31.2 | +01 11 25 | E2 | 15.4 | 14.4 | 0.9 × 0.7 | F, S, R, bMN | CGCG 391-39, NPM1G +01.0131 |
IC 2016 | 04 01 59.9 | +20 14 26 | S0 | 15.6 | 14.6 | 0.4 × 0.2 | eF, vS, * 15 s 30" | CGCG 466-6 |
IC 2019 1 | 04 01 53.7 | +05 38 21 | S | 15.3 | 14.5 | 0.8 × 0.4 | F, S, R, stell, r | UGC 2930, MCG 1-11-7, CGCG 418-7 |
IC 2019 2 | 04 01 52.7 | +05 38 10 | S | 15.3 | 14.5 | 0.3 × 0.2 | F, S, R, stell, r | UGC 2930, MCG 1-11-7, CGCG 418-7 |
IC 2057 | 04 21 56.0 | +04 02 53 | S? | 15.2 | 14.4 | 0.7 × 0.6 | pB, pS, R, gbM, r | CGCG 419-2, KARA 148, IRAS 04192+0355 |
PNG | RA J2000.0 | Dec J2000.0 | Main ID | PK | IRAS | Discoverer | Identities | oDiam ["] | rDiam ["] | Dist [kpc] | Rvel [km/s] | ExpVel [km/s] | C* Name | C* Mag | C* SP Type |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
PN G165.5-15.2 | 04 09 17 | +30 46 35 | NGC 1514 | 165-15.1 | 04061+3038 | PICKERING 1879 | ARO 21, VV 17, VV' 23 | 132. | 160. | 0.66 | +59.8 ± 4.4 | 25.0 (O-III) | AG +30 402, AG82 28, BD +30 623, FB 33, FB 34, HD 281679, PLX 915, SAO 57020 | U: 9.87, B: 9.93, V: 9.42 | sdO + A0 III |
PN G171.3-25.8 | 03 53 30 | +19 27 51 | Ba 1 | 171-25.1 | 03506+1920 | BAADE 1935 | ARO 87, VV 14, VV' 20 | 38. | -19.9 ± 8.6 | 35.5 (O-III) | AG82 24 | B: 18.7 | |||
PN G174.2-14.6 | 04 37 21 | +25 03 00 | H 3-29 | 174-14.1 | 04343+2456 | MAYALL 1964 | ARO 214 | 20. | 17. | -19.9 ± 2.0 | AG82 33, GL Tau | B: >18.8, V: >18.6 | |||
PN G181.5+00.9 | 05 52 48 | +28 06 26 | Pu 1 | PURGATHOFER 1978 | 65. | +38.6 ± 5.1 | AG82 50 | U: 20.58, B: 21.13, V: 21.16 | |||||||
PN G184.0-02.1 | 05 46 50 | +24 22 03 | M 1- 5 | 184-02.1 | 05437+2420 | MINKOWSKI 1946 | ARO 123, ARO 219, VV 24, VV' 35 | 2. | 2.3 | +37.4 ± 4.7 | 5.0 (O-III) | ||||
PN G184.6+00.6 | 05 58 45 | +25 18 44 | K 3-70 | 05556+2518 | KOHOUTEK 1969 | 1.8 | 1.5 | +26.9 ± 4.5 |