Sternbild Taurus (Stier)

Taurus
Taurus: IAU Sternbildkarte [150]

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
Daten für das Sternbild Taurus [150]
IAU NameTaurus
IAU GenitivTauri
IAU KürzelTau
Deutscher NameStier
Saison (47° N)August … März
Rektaszension03h 23m 21s … 06h 00m 55s
Deklination-01° 20' 46" … +31° 06' 01"
Fläche797 deg2
Nachbarn (N↻)Aur, Per, Ari, Cet, Eri, Ori, Gem

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:

Sternbild Taurus
Sternbild Taurus: Illustration aus «Uranometria» von Johann Bayer, Kupferstich von Alexander Mair, 1603 [28]

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]

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

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

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 1023BD+04 532210181111612509 Var?03 23 39.1+04 52 556.38 G5III 3.20.9S:Weak G-band.
HR 1028BD+12 47321051934162241 03 24 10.1+12 37 466.04 K0III-IV
HR 1030ο1BD+08 51121120111172121I 1134 03 24 48.8+09 01 443.60 G6IIIFe-1 SB:1654.9d, K 4.4k/s, V0 -20.1k/s, asini 96.7. Unresolved by speckle interferometry.
HR 1036BD+18 48421335934362242D 03 27 03.2+18 45 236.57 A3Vnp 0.00.1D: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 1038ξ2BD+09 43921364111195123 03 27 10.2+09 43 583.74 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 1039BD+12 4772137993439 03 27 18.7+12 44 066.28 A0V s
HR 10614BD+10 4522168693463 03 30 24.5+11 20 115.14 A0Vn
HR 1065BD+27 51521743759702582 A03 31 20.8+27 34 195.96 R A2V 0.411.4D:B CPM, A3V, vsini 100k/s, both components.
HR 10665BD+12 4862175493469125I 03 30 52.4+12 56 124.11 K0II-IIIFe-0.5 2.00.0SB: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 1067BD+05 502217551112302247 03 30 45.4+06 11 195.94 G8III
HR 10796BD+08 52821933111246 03 32 36.0+09 22 255.77 B9IV
HR 1085BD+17 5752207293494 03 34 08.3+17 49 586.17 K1IVFe-1
HR 10867BD+23 47322091759992616 1192 03 34 26.6+24 27 525.92 A3V+A3V 0.20.7D: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 1089BD+05 51122211111273 03 34 49.2+06 25 046.49 G0
HR 1099BD+00 616224681112912644 V711 Tau03 36 47.3+00 35 165.71 G9V 2.76.6D: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 110110BD-00 572224841112921101I 03 36 52.4+00 24 064.28 F9IV-V 10.0396.0D:CPM? Position angles disagree by about 40d.
HR 1102BD+14 5862252293524D 03 37 47.8+15 25 516.39 A5IV 0.00.1
HR 1103BD+20 6022261576045 1213 03 39 00.1+20 54 576.50 Am,A5-F0 G:Mel 22 #5006; Pleiades group.
HR 1110BD+16 484226959353622572661 03 39 25.7+16 32 126.16 K0III 0.00.3D:ADS 2661A, occultation double?, 7.1, 7.1v, sep. 0.3". Component B, 11.8v at 36" optical.
HR 111512BD+02 581227961113342258 03 39 51.1+03 03 255.57 gG6
HR 111811BD+24 52922805760731103D 03 40 46.3+25 19 466.11 A2IV 2.00.0G: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 1119BD-01 51922819130645 03 39 59.5-01 07 146.12 K1III-IV
HR 112613BD+19 57823016935572263 03 42 18.9+19 42 015.69 B9Vne S:Shell star. H alpha emission.
HR 113214BD+19 5822318393568 03 43 47.2+19 39 546.14 G8III G:61 Cyg group.
HR 1137BD+20 6212325876121 03 44 28.1+20 55 436.10 A0V
HR 114016BD+23 5052328876126D 1262 03 44 48.2+24 17 225.46 B7IV 2.00.0D: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 114217BD+23 5072330276131136D 03 44 52.5+24 06 483.70 B6III e2.00.0D: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 114418BD+24 5462332476137D 03 45 09.7+24 50 215.64 B8V 0.00.1G:Pleiades cluster; Mel 22 #541; embedded in reflection nebulosity.
HR 114519BD+24 5472333876140W 1264 03 45 12.5+24 28 024.30 B6IV 1.50.0D: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 114920BD+23 5162340876155D 1279 03 45 49.6+24 22 043.87 B8III v0.00.0C: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 115121BD+24 5532343276159 1283 03 45 54.4+24 33 175.76 B8V G:Pleiades cluster; Mel 22 #817.,N:Asterope. Sterope I.
HR 115222BD+24 5562344176164D 03 46 02.9+24 31 416.43 A0Vn 0.00.1D:Suspected occultation double.,G:Pleiades cluster; Mel 22 #859.,N:Sterope II.
HR 115329BD+05 5392346611140011042750 03 45 40.4+06 03 005.35 B3V 7.366.2D: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 115623BD+23 5222348076172W V971 Tau03 46 19.6+23 56 544.18 B6IVe vD: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 1159BD+06 58323526111407W 03 46 09.5+06 48 115.91 G9III
HR 1165η25BD+23 5412363076199139IW 03 47 29.1+24 06 182.87 B7IIIe 1.60.0C: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 1172BD+22 5632375376215D 1321 03 48 20.9+23 25 165.45 B8V 2.00.1G:Pleiades cluster; Mel 22 #1823.
HR 117430BD+10 48623793936112778 1327 03 48 16.3+11 08 365.07 B3V+F5V 4.49.2D:Binary.,G:Cas-Tau OB1.,M:Old disk population runaway star.,RV:Comp. B +17.2k/s; F5V or F3Vp.
HR 117827BD+23 55723850762281422786 1345 03 49 09.7+24 03 123.63 B8III 1.50.0D: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 118028BD+23 5582386276229 BU Tau03 49 11.2+24 08 125.09 B8Vpe vG: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 1183BD+23 5632392376244 03 49 43.5+23 42 426.17 B8V G:Pleiades cluster; Mel 22 #2425.
HR 1185BD+21 5352395076250 03 49 55.0+22 14 406.07 B8III G:Mel 22 #5025; Pleiades.,S:Spectra show Hg, Mn, Cr.
HR 1188BD+25 62423985762562799 1366 03 50 18.9+25 34 465.26 A2V+A5V 0.40.7D:5.81 A3V, 6.21 A5V, 62.28y, a = 0.430". Resolved by speckle interferometry 1983.93, sep. 0.66".
HR 1193BD+21 5392415476275D 03 51 36.6+22 01 546.83 R K0III D:Suspected occultation double.
HR 1194BD+12 5162415593637 V766 Tau03 51 15.8+13 02 456.30 B9pSi M:Old disk population runaway star.,VAR:Amp. 0.06y?, 2.53d.
HR 119931BD+06 594242631114692275W 03 52 00.2+06 32 055.67 B5V 0.10.6
HR 1201BD+16 52324357936501106 03 53 10.0+17 19 375.97 F4V G:In Taurus cluster; Mel 25 #6; the Hyades.
HR 121832BD+22 60524740763392283 03 56 52.1+22 28 415.63 F2IV
HR 122133BD+22 6072476976343D V817 Tau03 57 03.8+23 10 326.06 B9.5IV 2.00.0G: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 1222BD+24 5992480276350 03 57 26.4+24 27 436.16 K0
HR 1224BD+05 56424817111516 03 57 01.7+06 02 246.09 A2Vn
HR 1233BD+09 5242510293710 03 59 40.7+10 19 516.37 F5V G:In Taurus cluster; Mel 25 #8; the Hyades.
HR 1237BD+16 5442517593716 04 00 36.9+17 17 486.32 A0V
HR 1238BD+17 66625202937212288W 04 00 48.8+18 11 385.89 F4V 3.3164.2G:In Taurus cluster; Mel 25 #137; the Hyades.
HR 1239λ35BD+12 5392520493719150I Lam Tau04 00 40.8+12 29 253.47 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 1243BD+09 528253301115662938 04 01 46.1+09 59 525.67 B5V 5.212.0D:Component B, F8V, optical. Third component mag. diff 6.13v, at 100".
HR 1251ν38BD+05 58125490111579151 04 03 09.4+05 59 213.91 A1V
HR 125236BD+23 6092555576425I2965 04 04 21.7+24 06 215.47 G0III+A4V 0.00.0D: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 125340BD+05 58425558111585 04 03 44.6+05 26 085.33 B3V G:In HII region; Cas-Tau OB1.
HR 1254BD+07 59225570111586 04 03 56.6+08 11 505.46 F2V G:In Taurus cluster; Mel 25 #160; the Hyades.
HR 125637BD+21 58525604764301112IW 04 04 41.7+22 04 554.36 K0+III-IIIaFe-0.2 5.0137.2G:Hyades?
HR 1257BD+02 645256211115902292 04 04 09.9+02 49 375.36 F6IV G:Wolf 630 group.
HR 126239BD+21 5872568076438W 1452 04 05 20.2+22 00 325.90 G5V 2.7170.1G:Hyades?
HR 126841BD+27 6332582376455 GS Tau04 06 36.4+27 36 005.20 B9pSi vG: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 1269ψ42BD+28 61925867764612295 04 07 00.5+29 00 055.23 F1V
HR 1279BD+14 65726015937752999 1466 04 07 42.0+15 09 466.01 F3V 3.23.8D: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 1280BD+16 5602603893777I3006 04 07 59.4+17 20 235.89 K5IIIb 0.00.1D:Primary of ADS 3006 is occultation binary, sep. 0.05". Visual companion, 9.3v at 4.4", CPM.
HR 1283ω143BD+19 67226162937851115 04 09 10.0+19 36 335.50 K2III
HR 1284BD+13 64826171937842298 04 09 01.6+13 23 545.95 B9.5V
HR 128744BD+26 68626322764851116 IM Tau04 10 49.9+26 28 515.41 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 129245BD+05 601264621116482301W 04 11 20.3+05 31 235.72 F4V 4.1124.1G:In Taurus cluster; Mel 25 #14; the Hyades.
HR 1295BD+16 5692654693810 04 12 31.4+17 16 396.09 K0III
HR 1297BD+22 6492657176505 04 12 51.2+22 24 496.12 B9IIIp:Si: vVAR:Spectrum var.
HR 1307BD+09 5492667693821 04 13 34.8+10 12 446.23 B8Vn G:In reflection nebula; member assoc. Tau R2 at 135 pc.
HR 1308BD+08 651266771116713063 04 13 31.3+08 53 266.51 A2m 6.354.3D:B, 13.6v at 8"; C, optical.
HR 130946BD+07 617266901116723064 04 13 33.1+07 42 585.29 F2V+F5V 0.20.1D:6.0 F2V, 6.1 F3V, 7.18y, a = 0.135". Resolved by speckle interferometry 1983.93, sep. 0.09".,DYN:0.024".
HR 1310BD+12 5642670393823 04 13 49.9+12 45 126.25 K0 G:Probably Hyades group.
HR 131147BD+08 65226722111674I3072 04 13 56.4+09 15 494.84 G5III+A7V? 2.21.2D:AB binary; C, 12v at 32" optical.,DYN:0.003".,G:Hyades?
HR 1315BD+09 55026793111680 04 14 36.3+10 00 405.22 B9Vn
HR 131948BD+15 6032691193836W 1537 04 15 46.3+15 24 026.32 F5V 4.7151.4G:In Taurus cluster; Mel 25 #20; the Hyades.
HR 1320μ49BD+08 657269121116961118 04 15 32.1+08 53 324.29 B3IV G:Cas-Tau OB1; member of Pleiades group.
HR 1321BD+05 613269131116953085 BV891 Tau04 15 25.8+06 11 596.93 G5IV 0.664.7D: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 1322BD+05 614269231116983085 AV774 Tau04 15 29.2+06 11 126.31 G0IV 0.664.7D:CPM with HR 1321.,VAR:6.28 - 6.37V.
HR 1329ω250BD+20 7242704576532D Var?04 17 15.6+20 34 434.94 A3m 2.00.1D:Duplicity questioned.,SB:Over 5300d?, 5.0, 7.0v, sep. 0.05". Unresolved by speckle interferometry.
HR 133151BD+21 61827176765412313W 04 18 23.2+21 34 455.65 F0V 2.00.1D: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 1334BD+09 55827236111729 04 18 24.5+09 29 126.54 A4III
HR 133953BD+20 7332729576548 04 19 26.1+21 08 325.35 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 134156BD+21 6232730976551 V724 Tau04 19 36.7+21 46 255.38 A0pSi D:CPM with 1339.,G:Member of Pleiades group.,VAR:0.07V, 1.569d (light and spectrum).
HR 1346γ54BD+15 6122737193868159IS 1553 04 19 47.6+15 37 393.65 K0-IIIabCN1 G:In Taurus cluster; Mel 25 #28; the Hyades.,N:Hyadum I.,VAR:Amp. 0.1V.
HR 1348φ52BD+27 6552738276558I3137 04 20 21.3+27 21 034.95 K1III 3.750.0D:Optical.,G:Hyades?
HR 1349BD+09 5622738693866IA 04 19 37.5+10 07 176.31 K0 D:Astrometric binary unresolved by speckle interferometry.
HR 135157BD+13 6632739793872W V483 Tau04 19 57.7+14 02 075.59 F0IV 7.934.9D:Binary.,G:In Taurus cluster; Mel 25 #30; the Hyades.,VAR:Delta Sct 5.56 - 5.59V, 0.054d.
HR 1354BD+18 6242742993874 04 20 25.1+18 44 336.12 F3:V G:In Taurus cluster; Mel 25 #32; the Hyades.
HR 135658BD+14 6822745993876 V696 Tau04 20 36.3+15 05 435.26 F0V G:In Taurus cluster; Mel 25 #33; the Hyades.,VAR:Delta Sct 5.20 - 5.26V, 0.036d or double.
HR 1358BD+13 6652748393878 04 20 52.8+13 51 516.17 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 1360BD+05 631274971117562320 04 20 41.2+06 07 515.77 G8III-IV
HR 1361BD+08 67227505111759 04 20 49.0+09 13 326.53 A4V
HR 136860BD+13 6682762893892W V775 Tau04 22 03.5+14 04 385.72 A3m 7.1109.2G: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 1369χ59BD+25 70727638765733161 04 22 34.9+25 37 455.37 B9V 3.019.4D:CPM. Component A suspected occultation double; component B, G2V, strong lithium.,RV:ADS 3161B, +36.8k/s.
HR 1370BD+20 7442763976571I3158 04 22 22.8+20 49 175.91 M0IIIab+A,F 3.02.0DYN:0.003".
HR 1373δ161BD+17 7122769793897162IW 1582 04 22 56.1+17 32 333.76 K0-IIICN0.5 8.7109.6G: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 1375BD+20 7512774276585D 04 23 32.4+20 58 565.99 B8IV-V 0.00.2
HR 137663BD+16 5862774993900 Var?04 23 25.0+16 46 385.64 A1m 2.00.0G: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 137862BD+23 68427778765913179 A04 23 59.8+24 18 046.36 B3V 1.929.1D:AB CPM. B is A0. Component A suspected occultation double.,RV:ADS 3179B, +17.1k/s.
HR 1380δ264BD+17 7142781993907W 04 24 05.8+17 26 384.80 A7V 8.5143.0G:In Taurus cluster; Mel 25 #47; the Hyades.
HR 138166BD+09 570278201117913182 04 23 51.9+09 27 395.12 A3V 0.10.3D:5.8 A3V, 5.9 A4V, 51.6y, a = 0.18", or 55.40y, a = 0.20".,DYN:0.007".,G:UMa stream.
HR 1385BD+18 6332790193918 04 24 57.1+19 02 305.98 F4V G:In Taurus cluster; Mel 25 #53; the Hyades.
HR 1387κ165BD+21 64227934766013201 1593 04 25 22.1+22 17 384.22 A7IV-V 0.00.1D: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 1388κ267BD+21 64327946766023201 1594 04 25 25.0+22 11 595.28 A7V 0.00.1D:See HR 1387.,G:In Hyades cluster; Mel 25 #55.,VAR:Delta Sct, 5.26 - 5.29V.
HR 1389δ368BD+17 71927962939233206 V776 Tau04 25 29.4+17 55 414.29 A2IV 3.71.5D: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 139170BD+15 6212799193925W 04 25 37.3+15 56 276.46 F7V 0.00.1D: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 1392υ69BD+22 69628024766082326W Ups Tau04 26 18.5+22 48 494.28 A8Vn 1.90.0D: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 139471BD+15 6252805293932W V777 Tau04 26 20.8+15 37 064.49 F0V 2.00.1D: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 1396π73BD+14 6972810093935I 04 26 36.4+14 42 494.69 G7IIIaFe-1
HR 1397BD+08 687281141118172327 04 26 21.1+08 35 256.06 B6IV
HR 139972BD+22 6992814976613D 04 27 17.5+22 59 475.53 B7V N:On nomenclature see HR 1392.
HR 1400BD+01 75328191111827 04 27 00.7+02 04 466.23 K1III
HR 1402BD+10 57728217939433228 04 27 28.8+11 12 455.88 B8IV 1.80.4RV:Period possibly 19.83d or 20.43d.
HR 1403BD+21 6472822676618W 04 28 00.8+21 37 125.72 Am 0.80.0D: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 1406BD+30 66528271572493243 A04 28 51.9+30 21 416.40 F7V 1.814.7D:AB binary; C, 11.32V at 121" optical. Fourth component 13.3v at 17" from C.
HR 140775BD+16 6052829293950ID 1609 04 28 26.4+16 21 354.97 K2III v2.50.0D:Sep. 0.024".,R:Diam. 0.0020".
HR 140876BD+14 7022829493948 04 28 23.4+14 44 275.90 F0IV G:In Hyades cluster; Mel 25 #68.
HR 1409ε74BD+18 6402830593954164IW 04 28 37.0+19 10 493.53 G9.5IIICN0.5 7.0181.6G:In Hyades cluster; Mel 25 #70.,N:Ain; Oculus Boreus.
HR 1411θ177BD+15 6312830793955IW 04 28 34.5+15 57 443.84 K0IIIbFe-0.5 0.4337.4C: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 1412θ278BD+15 6322831993957W The2 Tau04 28 39.7+15 52 153.40 A7III 0.4337.4D: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 1413BD+01 75528322111840 04 28 03.6+01 51 316.15 G9III
HR 141479BD+12 59828355939602330 04 28 50.2+13 02 515.03 A7V G:Hyades cluster; Mel 25 #74.
HR 1415BD+01 757283751118451123 04 28 32.1+01 22 515.55 B3V N:44 Eri in Tau.
HR 1420BD+10 5832847593968 04 29 42.9+10 31 186.79 B5V
HR 142280BD+15 63628485939703264 04 30 08.6+15 38 175.58 F0V 2.21.7D: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 1425BD+09 5902850593971 04 30 02.4+10 15 456.48 G8III
HR 1427BD+15 6372852793975W 1627 04 30 33.7+16 11 384.78 A6IV 0.00.0D: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 142881BD+15 6392854693978W 04 30 38.9+15 41 315.48 A5m 3.9162.0G:In Hyades cluster; Mel 25 #83.
HR 143083BD+13 6902855693979W 04 30 37.3+13 43 285.40 F0V 5.8111.9G:In Hyades cluster; Mel 25 #84.
HR 143285BD+15 6452867793993 1640 04 31 51.8+15 51 066.02 F4V G:In Hyades cluster; Mel 25 #89.
HR 1436BD+05 67428736111879 04 32 04.8+05 24 366.39 F5V G:In Hyades cluster; Mel 25 #90.
HR 1442BD+17 75028867940023297 04 33 32.9+18 01 006.25 B9IVn 0.13.1D:Binary. No change after 113y.
HR 1444ρ86BD+14 72028910940071125 Rho Tau04 33 50.9+14 50 404.65 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 1445BD+28 66628929766543304 04 34 38.0+28 57 405.88 B9pHg 4.925.3S:Spectra show Hg; possibly Mn.
HR 1446BD+09 60028930111890 04 33 48.1+09 24 476.01 G8III
HR 1448BD+05 679289781118962335 04 34 08.3+05 34 075.68 A2V s G:In Ursa cluster; UMa stream.
HR 1455BD+19 74229104940223316 04 35 42.7+19 52 546.36 G5II-III+A-F 0.50.3D:Visual duplicity questioned. Unresolved by speckle interferometry 1983.93.
HR 1457α87BD+16 6292913994027168I3321 Alp Tau04 35 55.2+16 30 330.85 K5+III v9.8121.7D: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 145888BD+09 60729140940263317 1658 04 35 39.3+10 09 394.25 A5m 3.669.7D: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 1459BD+23 7152916976670 1663 04 36 29.2+23 20 276.02 F5IV G:In Taurus cluster; Mel 25 #100; the Hyades.
HR 1469BD+00 798293351119282339 1671 04 37 13.7+00 59 545.31 B7V N:49 Eri, in Tau.,VAR:5.3 - 5.38V.
HR 1470BD+26 73129364766823353 1676 04 38 29.6+26 56 246.47 R F2V: 0.14.0D:Occultation indicated mag. diff 0.37v, sep. 2.117" (half the visual sep.) and PA 78d in contrast to visual 194d.
HR 1471BD+20 78529365766802341 HU Tau04 38 15.8+20 41 055.92 B8V 1.50.0SB: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 147289BD+15 6612937594043W 04 38 09.4+16 02 005.79 F0V 5.9140.5G:In Taurus cluster; Mel 25 #103; the Hyades.
HR 147390BD+12 61829388940442342W 04 38 09.5+12 30 394.27 A6V 5.7119.8G:In Taurus cluster; Mel 25 #104; the Hyades.
HR 1477BD+24 67429459766892343 04 39 23.1+25 13 066.22 A5Vn
HR 1478σ191BD+15 6652947994051W 04 39 09.2+15 47 595.07 A4m 0.4431.2D: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 1479σ292BD+15 66629488940542345W 04 39 16.5+15 55 054.69 A5Vn 0.4431.2D:Binary with HR 1478.,G:Hyades cluster; Mel 25 #108.
HR 1480BD+07 681294991119542344W 04 39 06.2+07 52 155.39 A5m 3.5297.8G:In Taurus cluster; Mel 25 #107; the Hyades.
HR 148493BD+11 6392958994063 04 40 03.4+12 11 525.46 B8IV S:Spectra show Hg, Mn.
HR 1490BD+28 680296467670711263379 04 41 19.8+28 36 545.78 A2V 5.243.5D:AB, CPM. Third component by Wallenquist, mag. diff 6.42, sep. 90".
HR 1497τ94BD+22 7392976376721174W 04 42 14.7+22 57 254.28 B3V 0.70.1D: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 149995BD+23 7332985976727 04 43 13.8+24 05 206.13 F7IV-V
HR 1512BD+23 7393012276737 04 45 42.5+23 37 416.35 B5III G:Member of the local association (Pleiades group).
HR 1517BD+18 7193019794112 04 46 16.8+18 44 066.01 K4III G:Mel 25 #164; the Hyades, probable nonmember.
HR 153796BD+15 6873060594151I3464 04 49 44.1+15 54 156.08 gK3 5.529.3
HR 154797BD+18 74330780941641135W V480 Tau04 51 22.5+18 50 235.10 A7IV-V 5.3177.0G:In Hyades cluster; Mel 25 #123.,VAR:Delta Sct 5.09 - 5.11V, 0.042d.
HR 1554BD+27 70130912768022365 04 52 47.1+27 53 515.97 F2IV G:Hyades moving group.
HR 1566BD+19 8113123694199 04 54 58.3+19 29 076.37 F3IV G:In Taurus cluster; Mel 25 #126; the Hyades.
HR 1575BD+24 7093136276848 04 56 15.6+24 35 326.37 F0
HR 1585BD+16 6723153994227ID 04 57 22.3+17 09 135.48 gK1 0.00.1R:Diam. 0.0017".
HR 158699BD+23 77731553768583557 04 57 48.7+23 56 555.79 gG8 6.4103.5
HR 159098BD+24 717315927686223743547 04 58 09.4+25 03 015.81 A0V 5.894.6D:Component A suspected occultation double. Two visual companions.,RV:Two determinations of vsini, 170 and 50k/s.
HR 1620ι102BD+21 7513230176920184D 05 03 05.7+21 35 244.64 A7V 0.00.1D:Probable double, 5.4, 5.4v, sep. 0.4".,G:Hyades cluster; Mel 25 #129.
HR 1632BD+27 7233248076941 05 04 37.9+27 41 466.60 F0III
HR 1633BD+21 7553248276939 05 04 21.6+21 16 416.19 K0
HR 1642BD+19 84732642943063672 05 05 32.1+19 48 236.44 A5m 0.61.1
HR 1656104BD+18 77932923943323701 05 07 27.0+18 38 425.00 G4V 0.10.1D: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 1658106BD+20 88532977769712383 05 07 48.4+20 25 065.30 A5V G:Hyades?
HR 1659103BD+24 75532990769743709 05 08 06.6+24 15 555.50 B2V e5.735.3D: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 1660105BD+21 7663299176972W 05 07 55.5+21 42 175.89 B2Ve 0.00.3D: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 1670BD+27 732332047699011413730 A05 09 45.1+28 01 506.01 A5m 2.511.6D: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 1711108BD+22 8643405377057W 05 15 27.7+22 17 056.27 A2V 6.21.9
HR 1739109BD+21 81634559770972398I 05 19 16.6+22 05 474.94 G8III
HR 1741BD+19 89334579770983894 05 19 14.7+20 08 056.08 G8II-III+G1IV-V 3.59.0D:CPM. Companion 9.64V, +0.76(B-V), +0.19(U-B), G1IV-V.
HR 1750BD+27 7583476277121 05 20 59.3+27 57 266.33 B9IV 2.00.0SB:6.5, 8.5v, sep. 0.00002", 5.4337d, K 26.8k/s, V0 +5.8k/s, asini 2.00.
HR 1755BD+19 9023481094478 05 20 56.6+19 48 516.18 K0III
HR 1774110BD+16 7653518994514 05 23 37.7+16 41 586.08 A2IV
HR 1780111BD+17 9203529694526W 05 24 25.4+17 23 004.99 F8V 2.985.7D:Companion optical.
HR 1791β112BD+28 7953549777168202IW 05 26 17.5+28 36 271.65 B7III 33.4C: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 1798113BD+16 7753553294543 05 26 05.7+16 42 016.25 B2Vn
HR 1808115BD+17 928356719455411484038 05 27 10.1+17 57 445.42 B5V 1.20.1D: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 1810114BD+21 84735708771844048 05 27 38.1+21 56 134.88 B2.5IV 0.00.1D: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 1814116BD+15 8263577094566 05 27 45.6+15 52 275.50 B9.5Vn
HR 1816117BD+17 9313580294573I 05 28 01.6+17 14 205.77 M1III
HR 1821118BD+25 83935943772014068 A2009 05 29 16.5+25 09 025.47 B8.5V 0.84.8D:AB binary, B is A0V; colors for combined light. C, 11.5v at 141".,RV:ADS 4068B, +20k/s; vsini 197k/s.
HR 1831BD+22 9253616077220 05 30 43.4+22 27 456.29 K0
HR 1845119BD+18 8753638994628I CE Tau05 32 12.8+18 35 404.38 M2Iab-Ib eC:Large infrared excess.,R:Diam. 0.0105".,S:Ultraviolet FeII emission.,VAR:SRc 6.1 - 6.5p, 165d.
HR 1847BD+16 79436408946304131 A05 32 14.2+17 03 295.46 R B7IIIe 0.49.6D:Companion is B7IV, vsini 291k/s, optical.,SB:ADS 4131A.
HR 1858120BD+18 8773657694649 V960 Tau05 33 31.6+18 32 255.69 B2IV-Ve RV:Pole on?,S:Shell star.,VAR:Gamma Cas, 5.53 - 5.69V.
HR 1860BD+20 9893658977255 2132 05 33 38.8+20 28 276.18 B6V
HR 1875121BD+23 95436819772852415 Var?05 35 27.1+24 02 225.38 B2.5IV G:Member of the local association (Pleiades group); Cas-Tau OB1.,SB:7.83552d.
HR 1878BD+27 8063685977295I 05 35 55.5+27 39 446.27 K0
HR 1889BD+25 8793699477310 05 36 30.2+25 56 226.49 F5III
HR 1902BD+26 87037098773224208 2426 05 37 08.8+26 55 275.83 B9IV-V 0.11.1D:AB binary, both components B8IV. Combined magnitude and colors.
HR 1905122BD+16 8223714794700 05 37 03.8+17 02 255.54 F0V G:Mel 25 #168; Hyades cluster.
HR 1910ζ123BD+21 9083720277336211ID Zet Tau05 37 38.7+21 08 333.00 B4IIIpe v2.00.0C: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 1921BD+26 8843732977350D 05 38 57.4+26 37 046.37 R G9III D:Suspected occultation double.
HR 1928125BD+25 90237438773602424D 05 39 44.2+25 53 495.18 B3IV 2.00.0D: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 1929BD+21 9183743977358 05 39 27.0+21 45 466.34 R A1Vn
HR 1946126BD+16 84137711947594265 2560 05 41 17.7+16 32 024.86 B3IV 0.40.4D: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 1951BD+23 10073775277413 05 41 54.6+23 19 356.59 B8p S:Possibly Hg in spectrum.
HR 1954BD+22 9963778477420 05 42 03.9+22 39 376.36 R K2
HR 1961BD+23 10153796777450 V731 Tau05 43 19.5+23 12 156.21 B2.5Ve G:Cas-Tau OB1.,VAR:Amp. about 0.04V.
HR 1977BD+20 10833830777516I Y Tau05 45 39.4+20 41 426.95 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 1985129BD+15 9263847894848 05 46 45.5+15 49 216.00 B8IIIpHgMn:
HR 1989131BD+14 10253854594855 05 47 13.2+14 29 185.72 A3Vn
HR 1990130BD+17 10043855894858218 05 47 26.2+17 43 455.49 F0III
HR 1993133BD+13 979386229486424334381 05 47 42.9+13 53 595.29 B2IV-V 6.124.9D:Component B optical.,G:Member of the local association (Pleiades group); Cas-Tau OB1.
HR 1997BD+20 110538670775784392 05 48 22.4+20 52 106.07 B9Vn 1.40.5D:AB binary. C, 7.2v A0 at 75", CPM.,SB:ADS 4392A.
HR 2002132BD+24 97038751775922435ID 2650 05 49 01.0+24 34 034.86 G8III v0.00.1
HR 2010134BD+12 9123889994888W 05 49 32.9+12 39 044.91 B9IV 5.418.9
HR 2013BD+27 88839004776254474 05 50 58.1+27 58 045.56 gG7 1.30.0D:Third component, visual, 11.6v at 15". Reality of the occultation binary, sep. 0.01", has been questioned.,R:Occultation diam. = 0.0024".
HR 2016135BD+14 10413901994904 05 50 28.9+14 18 205.52 gG9
HR 2033137BD+14 10603931794945 V809 Tau05 52 22.3+14 10 185.59 B9pSiCrEu VAR:Amp. 0.05U, 2.63?d. Possible new periods of 2.654 and 1.5889d, of which the smaller preferred.
HR 2034136BD+27 89939357776751158D 2696 05 53 19.6+27 36 444.58 A0V 1.50.0SB:4.8, 6.3v, sep. 0.0013", 5.969d, K 48.9k/s, V0 -17.2k/s, msin3i 0.633, asini 4.01.
HR 2074BD+24 10333997077750 05 56 56.1+24 14 596.02 A0Ia G:Gem OB1.
HR 2084139BD+25 10524011177775 05 57 59.7+25 57 144.82 B0.5II C:Color excess E(B-V) = +0.15.,G:Gem OB1.,S:uv indicates gB0.5.

Revised+Historic NGC/IC, Version 22/9, © Dr. Wolfgang Steinicke [277]
Planetarische Nebel
NameRADecTypbMagvMagDimDreyer BeschreibungIdentifikation, Anmerkungen
NGC 151404 09 17.0+30 46 35PN10.010.92.2* 9m in neb 3' diamPK 165-15.1, CS=9.4
Galaktische Nebel
NameRADecTypbMagvMagDimDreyer BeschreibungIdentifikation, Anmerkungen
NGC 143203 45 49.5+24 22 06RN26 × 26eF, vL, dif (Maja Plejadum)LBN 772, Maia nebula
NGC 143503 46 10.0+23 45 54RN30 × 30vF, vL, dif (Merope)CED 19I, Merope nebula
NGC 155504 21 56.7+19 32 04RN0.5!!! vF, S, variable (Auw 20)DG 31, CED 32B, vdB 28, Hind's variable nebula
NGC 195205 34 31.9+22 00 52SNR8.46 × 4vB, vL, E 135° ±, vglbM, rM 1, LBN 833, Sh2-244, CED 53, Taurus A, Crab nebula
IC 33603 37 00.0+23 24 00ENvF, eeL, v dif
IC 34103 40 00.0+22 00 00EN135vF, eeL, v difCED 19B
IC 34903 46 20.0+23 56 23RN0.5 × 0.5eF, vS, Pos. 165°, Dist. 36" from MeropeCED 19I, Barnard's Merope nebula
IC 35303 53 00.3+25 48 00EN180 × 30vF, eeL, v difLBN 601, Ced 24
IC 35403 53 00.0+23 00 00EN130vF, eeL, v difCED 19q
IC 36004 09 00.0+26 06 00EN180 × 100vF, eeL, v difLBN 786
IC 199003 47 13.8+24 20 02ENvL, mE pf, 15' lCED 19M
IC 199503 50 18.5+25 34 51RN135 × 135* 6 in eF, eeL neb (M.N., lx. P. 260)CED 22, Pos of SAO 76256
IC 208704 40 00.0+25 44 32RN4 × 4eeF, in hole of eL nebyLBN 813, CED 38
IC 208804 31 00.0+26 36 00EN360eeL, 3° longLBN 793
IC 214405 50 14.0+23 52 20EN1pF, eS, * 12 nnp 2', * 12 s 1'BFS 50
Offene Sternhaufen
NameRADecTypbMagvMagDimDreyer BeschreibungIdentifikation, Anmerkungen
NGC 164704 45 42.2+19 07 09II2m6.440Cl, vL, st L, scOCL 457
NGC 175005 03 54.0+23 39 30OCL25 × 12Cl, st L, vc scOCL 454
NGC 175805 04 36.0+23 47 54IV1p40Cl, pC, st L and SOCL 453
NGC 180205 10 14.0+24 07 30OCL20Cl, st c sc*Grp ?
NGC 180705 10 46.0+16 30 48II2p7.012Cl, pRi, st L & SOCL 462, * group?
NGC 181705 12 27.0+16 41 00III1m7.720Cl, L, Ri, lC, st 11…14OCL 463
NGC 202605 43 12.0+20 08 00OCL10Cl, lRi, lC, st pL
Galaxien
NameRADecTypbMagvMagDimDreyer BeschreibungIdentifikation, Anmerkungen
NGC 134903 31 27.4+04 22 53S014.213.10.8 × 0.8eeF, S, R, bet 2 stUGC 2774, MCG 1-9-6, CGCG 416-13, KARA 128, NPM1G +04.0118
NGC 138403 39 13.5+15 49 10Sc15.214.50.9 × 0.5Neb * 13MCG 3-10-3, CGCG 465-4
NGC 140903 41 10.4-01 18 07SB014.813.81 × 0.8eF, stellar or lEUGC 2821, MCG 0-10-11, CGCG 391-28, KCPG 93A, VV 729, 3ZW 55, NPM1G -01.0133
NGC 141003 41 10.8-01 17 55E115.014.00.7 × 0.6Makes D neb with h 304, pos 0°UGC 2821, MCG 0-10-12, CGCG 391-28, KCPG 93B, VV 729, 3ZW 55
NGC 143103 44 40.7+02 50 08S015.114.11 × 0.8eF, pL, iRUGC 2845, MCG 0-10-17, CGCG 391-33, NPM1G +02.0129
NGC 146203 50 23.4+06 58 23S15.214.40.9 × 0.5vF, S, vlEMCG 1-10-10, CGCG 417-7
NGC 147403 54 30.3+10 42 25SBa14.713.81.1 × 1vF, S, RIC 2002, UGC 2898, MCG 2-10-3, CGCG 442-5, KARA 135
NGC 149704 02 06.8+23 08 00S014.113.11.5 × 0.7eF, vS, iR, mbMUGC 2929, MCG 4-10-8, CGCG 487-9, NPM1G +22.0134
NGC 150804 05 47.6+25 24 33Sc15.214.50.7 × 0.6vF, vS, R, bM, rMCG 4-10-21, CGCG 487-21, NPM1G +25.0119
NGC 151704 09 11.9+08 38 56Sc14.113.41.1 × 1vF, vS, R, r, * 9, 10 sfUGC 2970, CGCG 418-13, IRAS 04064+0831
NGC 1539 104 19 01.9+26 49 39C15.814.80.5 × 0.5vF, vS, gbMCGCG 488-1, 5ZW 373
NGC 1539 204 19 02.7+26 49 46C17.616.60.3 × 0.3vF, vS, gbMCGCG 488-1, 5ZW 373
NGC 154104 17 00.2+00 50 07S0-a14.613.61.3 × 0.5vF, SUGC 3001, MCG 0-11-40, CGCG 392-13
NGC 154204 17 14.1+04 46 55Sab14.713.91.3 × 0.5vF, S, EUGC 3003, MCG 1-11-16, CGCG 418-17, KARA 145, IRAS 04145+0439
NGC 155104 19 38.1+02 24 34E-S013.112.02.2 × 1.9F, vS, R, probably = 835NGC 1550, UGC 3012, MCG 0-11-55, CGCG 393-1
NGC 158704 30 40.0+00 39 45E212.711.71.7 × 1.4F, pS, R, r, p of D nebUGC 3063, MCG 0-12-35, CGCG 393-28, KCPG 99A, 2ZW 12
NGC 158804 30 43.7+00 39 55E513.912.91.1 × 0.6F, vS, R, r, f of D nebUGC 3064, MCG 0-12-37, CGCG 393-29, KCPG 99B, MK 616, 2ZW 12, NPM1G +00.0155
NGC 158904 30 45.4+00 51 48Sab12.811.83.2 × 1F, pL, lE 132°, * 42°, 80"UGC 3065, MCG 0-12-38, CGCG 393-30
NGC 159004 31 10.2+07 37 51S/P14.513.70.9 × 0.7F, S, * 12 nfUGC 3071, MCG 1-12-8, CGCG 419-14, IRAS 04284+0731, 2ZW 13, KUG 0428+075
NGC 159304 32 06.1+00 34 04S014.413.41.6 × 0.6vFNGC 1608, IC 2077, UGC 3082, MCG 0-12-44, CGCG 393-37, NPM1G +00.0156
NGC 161504 36 01.9+19 57 03E-S014.613.91.2 × 0.8vF, vS, R, lbM, vS * invUGC 3096, MCG 3-12-5, CGCG 467-3
NGC 163304 40 09.1+07 20 59SBab14.313.51 × 0.9eF, S, R, * 8 sp, p of D nebUGC 3125, MCG 1-12-14, CGCG 419-23, KCPG 101A
NGC 163404 40 09.8+07 20 20E-S015.114.10.4 × 0.3eF, vS, f of D nebMCG 1-12-15, CGCG 419-22, ARAK 109, KCPG 101B
NGC 164204 42 54.9+00 37 08Sc13.312.61.7 × 1.2F, R, Cometary, Δ with 2 st 18, fUGC 3140, MCG 0-12-72, CGCG 393-73, IRAS 04403+0031
IC 32203 26 00.5+03 40 49D15.214.60.9 × 0.8vF, pL, vlbM, difficCGCG 390-89, CGCG 416-8
IC 32903 32 01.3+00 16 48S?15.214.30.9 × 0.4F, vS, R, lbMMCG 0-10-1, CGCG 391-2, NPM1G +00.0135
IC 33003 32 07.9+00 21 12Sab14.914.11.2 × 0.3F, vS, R, lbMUGC 2779, MCG 0-10-2, CGCG 391-4
IC 33103 32 19.0+00 16 58S14.713.90.9 × 0.9* 13 in nebMCG 0-10-3, CGCG 391-5, IRAS 03296+0005
IC 33203 32 37.4+01 22 59S0-a14.613.70.9 × 0.5F, vS, R, sbMMCG 0-10-4, CGCG 391-6, KARA 129, NPM1G +01.0123
IC 33803 37 38.1+03 07 06S?14.713.80.8 × 0.7vF, S, dif, vF * closeMCG 0-10-7, CGCG 391-18
IC 35503 53 46.3+19 58 27Sc15.614.90.5 × 0.5vF, S, R, difMCG 3-10-10, CGCG 465-10, IRAS 03509+1949
IC 35704 03 43.9+22 09 35SBab14.013.21.2 × 1F, S, R, N = 13.5UGC 2941, MCG 4-10-16, CGCG 487-16, NPM1G +22.0137, IRAS 04007+2201
IC 35804 03 42.8+19 53 44S015.114.11 × 0.4vS, dif, lbMUGC 2940, MCG 3-11-6, CGCG 466-9, NPM1G +19.0125
IC 35904 12 28.4+27 42 11E-S014.913.91.3 × 1.3eeF, pL, RUGC 2980, MCG 5-10-9, CGCG 508-8
IC 36304 18 55.2+03 01 56C15.414.40.2 × 0.2eF, * 9 nf 3'CGCG 392-19
IC 36404 19 06.6+03 11 22E514.813.80.4 × 0.2vF, vS, R, sbMCGCG 392-20, NPM1G +03.0150
IC 36504 19 14.2+03 20 56S0-a14.813.91 × 0.6pB, S, iF, sbMMCG 1-11-17, CGCG 392-21, IRAS 04166+0313
IC 36604 19 41.5+02 21 37E315.714.70.3 × 0.2eF, 3' sf of 1550CGCG 393-2, NPM1G +02.0138
IC 37404 32 32.8+16 38 06S15.714.90.8 × 0.4F, S, R, mbMMCG 3-12-1, CGCG 467-1, ARAK 107
IC 38304 38 58.0+09 53 33E015.814.80.4 × 0.4vF, S, dif, * 11.5 f
IC 191803 26 17.8+04 32 30S14.914.10.4 × 0.2F, S, glbM, difCGCG 416-9, NPM1G +04.0115
IC 193003 28 46.1+04 23 02E316.015.00.4 × 0.3F, S, R, gbM, * 8 p 3s, s 1'.6
IC 193103 28 57.8+01 45 02D15.314.70.8 × 0.8vF, difMCG 0-9-87, CGCG 390-94
IC 195603 35 33.2+05 04 02SBbc15.414.61.6 × 0.3F, S, E 200°, 2 vF NucleiUGC 2795, MCG 1-10-1, CGCG 417-1, KARA 130, IRAS 03329+0454
IC 196703 37 47.8+03 16 13S?15.815.00.9 × 0.4vF, S, R, * 13 nrMCG 0-10-8, CGCG 391-20, IRAS 03351+0306
IC 197703 40 45.0+17 44 27SBb14.313.51.4 × 0.8F, S, R, dif, * 13.5 nrUGC 2815, MCG 3-10-5, CGCG 465-7, IRAS 03378+1734
IC 199803 51 31.2+01 11 25E215.414.40.9 × 0.7F, S, R, bMNCGCG 391-39, NPM1G +01.0131
IC 201604 01 59.9+20 14 26S015.614.60.4 × 0.2eF, vS, * 15 s 30"CGCG 466-6
IC 2019 104 01 53.7+05 38 21S15.314.50.8 × 0.4F, S, R, stell, rUGC 2930, MCG 1-11-7, CGCG 418-7
IC 2019 204 01 52.7+05 38 10S15.314.50.3 × 0.2F, S, R, stell, rUGC 2930, MCG 1-11-7, CGCG 418-7
IC 205704 21 56.0+04 02 53S?15.214.40.7 × 0.6pB, pS, R, gbM, rCGCG 419-2, KARA 148, IRAS 04192+0355

«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 G165.5-15.204 09 17+30 46 35NGC 1514165-15.104061+3038PICKERING 1879ARO 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 57020U: 9.87, B: 9.93, V: 9.42sdO + A0 III
PN G171.3-25.803 53 30+19 27 51Ba 1171-25.103506+1920BAADE 1935ARO 87, VV 14, VV' 20 38. -19.9 ± 8.6 35.5 (O-III)AG82 24B: 18.7
PN G174.2-14.604 37 21+25 03 00H 3-29174-14.104343+2456MAYALL 1964ARO 214 20. 17. -19.9 ± 2.0AG82 33, GL TauB: >18.8, V: >18.6
PN G181.5+00.905 52 48+28 06 26Pu 1PURGATHOFER 1978 65. +38.6 ± 5.1AG82 50U: 20.58, B: 21.13, V: 21.16
PN G184.0-02.105 46 50+24 22 03M 1- 5184-02.105437+2420MINKOWSKI 1946ARO 123, ARO 219, VV 24, VV' 35 2. 2.3 +37.4 ± 4.7 5.0 (O-III)
PN G184.6+00.605 58 45+25 18 44K 3-7005556+2518KOHOUTEK 1969 1.8 1.5 +26.9 ± 4.5

Quellenangaben

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
20«Sternbilder und ihre Mythen» von Gerhard Fasching; Zweite, verbesserte Auflage; Springer Verlag Wien, New York; ISBN 3-211-82552-5 (Wien); ISBN 0-387-82552-5 (New York)
28«Uranometria omnium asterismorum continens schemata, nova methodo delineata aereis laminis expressa» Johann Bayer, Augsburg, 1603; DOI:10.3931/e-rara-309
77The Starry Sky: Taurus by Deborah Byrd; Astronomy 12/94, p.60
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)