Kataloge

Katalog

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Taurus / Yale Bright Star Catalog (HR)

«Yale Bright Star Catalogue, 5th Revised Ed.» Hoffleit D., Warren Jr W.H., 1991 ^[154]
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.

Legende

Key to columns ^[154]
HR	Harvard Revised Number = Bright Star Number
B	Bayer designation (greek letter)
F	Flamsteed number
DM	Durchmusterung Identification (BD = Bonn; CD = Cordoba; CP = Cape Photographic)
HD	Henry Draper Catalog Number
SAO	SAO Catalog Number
FK5	FK5 star Number
IR	I if infrared source
M*	Double or multiple-star code. (A = Astrometric binary; D = Duplicity discovered by occultation; I = Innes, Southern Double Star Catalogue (1927); R = Rossiter, Michigan Publ. 9, 1955; S = Duplicity discovered by speckle interferometry; W = Worley (1978) update of the IDS;)
ADS	Aitken's Double Star Catalog (ADS) designation
VarID	Variable star identification
RA	Right Ascension (J2000.0)
Dec	Declination (J2000.0)
vMag	Visual magnitude
spType	Spectral type
dMag	Magnitude difference of double, or brightest multiple
Sep	Separation of components in Dmag if occultation binary (arcsec)
Remarks	Note on Category (C = Colors; D = Double and multiple stars; DYN = Dynamical parallaxes; G = Group membership; M = Miscellaneous; N = Star names; P = Polarization; R = Stellar radii or diameters; RV = Radial and/or rotational velocities; S = Spectra; SB = Spectroscopic binaries; VAR = Variability)

Kataloge

Taurus / Yale Bright Star Catalog (HR)

Legende

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