1979A&A....78..292K

Query : 1979A&A....78..292K

1979A&A....78..292K - Astronomy and Astrophysics, volume 78, 292-298 (1979)

Apparent spectral inconsistencies due to the gravity darkening of pole-on rapidly-rotating B-type stars.

KODAIRA K. and HOEKSTRA R.

Journal keyword(s):

Simbad objects: 34

goto View the references in ADS

Number of rows : 34
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024 		#notes
1 * gam Peg bC* 00 13 14.1523490172 +15 11 00.954346538 1.75 2.61 2.84 2.94 3.13 B2IV 693 0
2 * zet Cas bC? 00 36 58.2844874846 +53 53 48.877599163 2.58 3.47 3.66 3.74 3.95 B2IV 453 0
3 * del Cet bC* 02 39 28.9568473856 +00 19 42.631195332 2.97 3.85 4.07     B2IV 380 0
4 * lam Tau EB* 04 00 40.8167738514 +12 29 25.239987626 2.66 3.29 3.41 3.44 3.53 B4IV 349 0
5 * eta Aur PM* 05 06 30.8941413263 +41 14 04.112669983 2.33 3.00 3.18 3.23 3.40 B3V 377 0
6 * zet CMa Ce* 06 20 18.7920398 -30 03 48.120242 2.12 2.82 2.99     B2.5V 162 0
7 * chi Car bC* 07 56 46.7200933968 -52 58 56.443666728 2.64 3.267 3.431     B3IV 148 1
8 * eta Hya bC* 08 43 13.4757536071 +03 23 55.182801587 3.380 4.100 4.300 4.37 4.56 B3V 405 1
9 * kap Vel SB* 09 22 06.8176100 -55 00 38.401683 1.5 2.324 2.473     B2IV 164 0
10 * del Cru Pu* 12 15 08.7184790676 -58 44 56.126676618 1.63 2.568 2.752     B2IV 212 1
11 * sig Cen ** 12 28 02.3821158564 -50 13 50.296708174 2.95 3.72 3.91 4.02 4.22 B2V 161 0
12 * alf Mus ** 12 37 11.0178886 -69 08 08.033239 1.62 2.484 2.649     B2IV 150 1
13 * eta UMa PM* 13 47 32.43776 +49 18 47.7602 0.99 1.67 1.86 1.98 2.16 B3V 608 0
14 * nu. Cen bC* 13 49 30.2765077433 -41 41 15.750707249 2.31 3.188 3.386     B2V 198 0
15 * ups01 Cen Pu* 13 58 40.7486851 -44 48 12.908967 2.87 3.67 3.87 4.01 4.22 B2IV-V 148 0
16 * iot Lup V* 14 19 24.2211609376 -46 03 29.139332461 2.65 3.355 3.529     B2.5IV 112 0
17 * b Cen ** 14 41 57.5905450998 -37 47 36.580200460 3.14 3.83 4.00 4.11 4.26 B2.5V 145 0
18 * bet Lup PM* 14 58 31.92536 -43 08 02.2699 1.59 2.46 2.68 2.78 2.95 B2III 188 0
19 * kap Cen bC* 14 59 09.6849382 -42 06 15.106919 2.15 2.93 3.11     B2IV 203 0
20 * del Lup bC* 15 21 22.3138254072 -40 38 51.109328940 2.12 2.995 3.190     B1.5IV 220 0
21 * eps Lup bC* 15 22 40.8682566 -44 41 22.614637 2.46 3.191 3.366     B3IV+B3:V 181 0
22 * gam Lup El* 15 35 08.44835 -41 10 00.3247 1.76 2.586 2.765     B2IV 178 0
23 * tau Lib SB* 15 38 39.3694957 -29 46 39.895604   3.481 3.642     B2.5V 158 0
24 * eta Lup bC? 16 00 07.3279160436 -38 23 48.138224969 2.36 3.19 3.41     B2.5IV 166 0
25 * tet Lup Pu* 16 06 35.5439828160 -36 48 08.173906632 3.36 4.027 4.201     B2.5Vn 118 0
26 * nu. Sco ** 16 11 59.73568 -19 27 38.5361 3.42 4.05 4.00 3.90 3.87 B2V 381 0
27 * tet Oph bC* 17 22 00.5793468 -24 59 58.366974 2.18 3.03 3.26 3.38 3.58 OB 332 0
28 * ups Sco * 17 30 45.8371228 -37 17 44.928511 1.64 2.48 2.65     B2IV 184 0
29 * lam Sco bC* 17 33 36.52012 -37 06 13.7648 0.52 1.49 1.63     B2IV+DA7.9 391 0
30 * iot Her bC* 17 39 27.8868980278 +46 00 22.792978043 2.940 3.630 3.800     B3IV 448 1
31 * kap Sco bC* 17 42 29.27520 -39 01 47.9391 1.32 2.211 2.386     B1.5III 241 0
32 * alf Tel PM* 18 26 58.4164240310 -45 58 06.447916980 2.7 3.299 3.463     B3IV 139 0
33 * sig Sgr ** 18 55 15.92650 -26 17 48.2068 1.06 1.923 2.067     B2.5V 269 1
34 * alf Pav SB* 20 25 38.85705 -56 44 06.3230 1.03 1.791 1.918     B2IV 292 1

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