1990ApJS...73..461S

Query : 1990ApJS...73..461S

1990ApJS...73..461S - Astrophys. J., Suppl. Ser., 73, 461-480 (1990/May-0)

A multiwavelength study of the Carlson-Henize sample of early-type galactic extreme emission-line stars.

SHORE S.N., BROWN D.N., BOPP B.W., ROBINSON C.R., SANDULEAK N. and FELDMAN P.D.

Abstract (from CDS):


Abstract Copyright: ∼

Journal keyword(s): Stars: Be - Stars: Supergiants - Ultraviolet: Spectra

Simbad objects: 30

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Number of rows : 30
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 * kap Cas s*b 00 32 59.9918836206 +62 55 54.413126128 3.50 4.30 4.16 4.02 3.96 BC0.7Ia 474 0
2 CPD-75 116 s*b 01 44 03.8703845040 -74 40 49.800525744   11.54 11.43 11.69   B5Ia[e] 92 0
3 * 10 Per s*b 02 25 16.0283450208 +56 36 35.354429280 5.95 6.56 6.26 5.93 5.74 B2Ia 248 0
4 * alf Cam s*b 04 54 03.0113886719 +66 20 33.633625509 3.47 4.34 4.29 4.18 4.18 O9Ia 675 1
5 HD 34664 s*b 05 13 52.9937299920 -67 26 54.820789332 11.509 11.88 11.774 11.63 10.991 B0/0.5I[e] 103 0
6 * eps Ori s*b 05 36 12.81335 -01 12 06.9089 0.48 1.51 1.69 1.76 1.93 B0Ia 921 0
7 HD 37974 s*b 05 36 25.8534763728 -69 22 55.789571064 10.056 11.12 10.99 11.00 10.423 B0.5e 132 0
8 HD 269858 s*b 05 36 43.6936418088 -69 29 47.451149232   10.24 10.15 9.95 9.05 LBV 296 2
9 * chi02 Ori s*b 06 03 55.1843706432 +20 08 18.428141364 4.24 4.91 4.63 4.32 4.10 B2Ia 465 0
10 * 3 Gem s*b 06 09 43.9852949424 +23 06 48.472220448 5.33 5.96 5.75     B2.5Ib 234 0
11 WRAY 15-30 LP* 07 31 40.7186605632 -41 35 20.798911392   13.06 12.38 12.08 10.03 ~ 12 0
12 * l Pup sg* 07 43 48.4696146486 -28 57 17.374357218 4.06 4.09 3.93 3.68 3.50 A4Iabe 201 0
13 HD 74371 s*b 08 41 56.9097314184 -45 24 38.562399648 4.94 5.378 5.227 6.75   B6Iab/b 98 0
14 HD 80558 s*b 09 18 42.3559197816 -51 33 38.338564212 6.15 6.47 5.93 5.36 4.94 B6Ia 124 0
15 HD 87643 Or* 10 04 30.2839505304 -58 39 52.091224848 8.92 10.38 9.50 9.68   B3I[e] 157 0
16 HD 89249 Be* 10 16 20.6463551616 -55 35 51.316367604 8.98 9.51 9.10 9.26   Bp_sh 46 0
17 HD 90177 s*b 10 22 53.8430096928 -59 37 28.363616256 9.16 9.66 8 8.15   LBV 342 0
18 HD 100198 sg* 11 31 15.0458770704 -61 16 42.487275684 6.75 6.90 6.40 5.84 5.45 A3Ia 59 0
19 MR 41 WR* 12 11 18.5515062048 -62 29 43.613827440   12.24 11.35 10.94 9.78 WR 22 0
20 HD 115842 s*b 13 20 48.3393402216 -55 48 02.482824528 5.70 6.39 6.09 5.77 5.52 B0.5Ia 162 0
21 CPD-52 9243 AB* 16 07 02.0298241344 -53 03 45.415519128 12.36 11.84 10.22 9.87   B3Ieq 62 0
22 HD 149404 s*b 16 36 22.5628499784 -42 51 31.902127776 5.23 5.88 5.52 6.90   O8.5Iab(f)p 265 0
23 HD 151932 WR* 16 52 19.2477039480 -41 51 16.270066224 6.06 6.79 6.51 7.64   WN7h 326 0
24 HD 152235 s*b 16 53 58.8528412848 -41 59 39.577848180 6.47 6.92 6.38 5.84 5.42 B0.5Ia 205 0
25 CD-42 11721 Be* 16 59 06.7629322176 -42 42 08.404228224 12.16 12.28 11.00     B0IVe 179 0
26 HD 326823 WR* 17 06 53.9045282184 -42 36 39.704037840 9.68 9.87 9.03 9.51   WNpec 83 1
27 HD 316285 s*b 17 48 14.0372119152 -28 00 53.121269592 11.88 11.27 9.60 9.28   B0Ieq 197 2
28 * mu. Sgr s*b 18 13 45.8088401 -21 03 31.794073 3.60 4.07 3.85 3.58 3.38 B8Iab(e) 354 0
29 * P Cyg s*b 20 17 47.2019733389 +38 01 58.549132671 4.66 5.24 4.82 4.28 4.02 B1-2Ia-0ep 1200 1
30 * 6 Cas ** 23 48 50.17052 +62 12 52.2577       6.60   A2.5(I)+O9.8II 199 0

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