1990MNRAS.246..408P

Query : 1990MNRAS.246..408P

1990MNRAS.246..408P - Mon. Not. R. Astron. Soc., 246, 408 (1990)

Intrinsic energy distributions in spectra of early-type stars.

PAPAJ J., WEGNER W. and KRELOWSKI J.

Journal keyword(s):

Simbad objects: 35

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Number of rows : 35
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 * del Cet bC* 02 39 28.9568473856 +00 19 42.631195332 2.97 3.85 4.07     B2IV 380 0
2 * nu. Eri bC* 04 36 19.1419185396 -03 21 08.857744927 2.82 3.737 3.928     B2III 390 0
3 * psi Eri * 05 01 26.3457823592 -07 10 26.273231188 3.87 4.62 4.81     B3IV 108 0
4 * lam Lep * 05 19 34.5223081894 -13 10 36.369844928 3.03 4.04 4.29 4.41 4.69 B0.5V 302 0
5 * ups Ori SB* 05 31 55.8599595648 -07 18 05.535884975 3.30 4.36 4.63 4.75 5.01 O9.7V 408 0
6 HD 36960 * 05 35 02.6823091513 -06 00 07.308349203 3.52 4.50 4.72     B0.5V 268 0
7 * iot Ori SB* 05 35 25.9819073 -05 54 35.643537 1.45 2.53 2.77     O9IIIvar 773 0
8 * eps Ori s*b 05 36 12.81335 -01 12 06.9089 0.48 1.51 1.69 1.76 1.93 B0Ia 896 0
9 * zet Ori A SB* 05 40 45.527143 -01 56 33.26036   1.79 1.90     O9.2IbvarNwk 666 0
10 HD 37756 SB* 05 40 50.7155671106 -01 07 43.635084978 3.91 4.74 4.95     B3V 140 0
11 * mu. Col V* 05 45 59.8950238944 -32 18 23.162261796 3.84 4.90 5.18 5.30 5.57 O9.5V 495 0
12 * kap Ori s*b 05 47 45.3888404 -09 40 10.577707 0.87 1.88 2.06 2.09 2.27 B0.5Ia 569 0
13 HD 43112 * 06 15 08.4727512648 +13 51 03.959285616 4.7 5.676 5.894     B1V 118 0
14 * lam CMa * 06 28 10.2080207479 -32 34 48.246033640 3.70 4.31 4.48 4.54 4.70 B4V 80 0
15 HD 48402 * 06 40 47.4509196144 -47 37 17.467404132 5.97 6.502 6.629     B3/5V 40 0
16 * kap CMa Be* 06 49 50.4591124672 -32 30 30.523820933 2.73 3.68 3.89 3.91 4.05 B1.5Ve 286 0
17 * 42 Cam * 06 50 57.0890928144 +67 34 18.963203232 4.32 4.961 5.122     B4IV 72 0
18 HD 51925 ** 06 58 07.5533495 -27 09 51.781515 5.32 6.181 6.361     B2V 48 0
19 * y Pup XB* 07 29 05.6951953008 -38 48 43.442359164   5.243 5.395     B3V 84 0
20 HD 64740 * 07 53 03.6344819483 -49 36 46.956285817 3.48 4.40 4.63 4.76 4.97 B2V 211 0
21 * eta Hya bC* 08 43 13.4757536071 +03 23 55.182801587 3.380 4.100 4.300 4.37 4.56 B3V 405 1
22 * f Vel EB* 08 50 33.4606230120 -46 31 45.075306720 3.92 4.90 5.11 5.20 5.36 B1Ib 160 0
23 HD 96088 * 11 04 00.2319399264 -57 57 19.217568888 5.16 5.96 6.13     B2III 39 0
24 * eta UMa PM* 13 47 32.43776 +49 18 47.7602 0.99 1.67 1.86 1.98 2.16 B3V 608 0
25 * nu. Cen bC* 13 49 30.2765077433 -41 41 15.750707249 2.31 3.188 3.386     B2V 198 0
26 * bet Lup PM* 14 58 31.92536 -43 08 02.2699 1.59 2.46 2.68 2.78 2.95 B2III 188 0
27 * del Lup bC* 15 21 22.3138254072 -40 38 51.109328940 2.12 2.995 3.190     B1.5IV 220 0
28 * eta Lup bC? 16 00 07.3279160436 -38 23 48.138224969 2.36 3.19 3.41     B2.5IV 166 0
29 * bet01 Sco bC* 16 05 26.2319826 -19 48 19.630018 1.68 2.55 2.62 2.60 2.69 B1V 561 0
30 * tau Sco * 16 35 52.9528530 -28 12 57.661515 1.55 2.56 2.81 2.93 3.18 B0.2V 920 0
31 * tet Oph bC* 17 22 00.5793468 -24 59 58.366974 2.18 3.03 3.26 3.38 3.58 OB 332 0
32 * kap Sco bC* 17 42 29.27520 -39 01 47.9391 1.32 2.211 2.386     B1.5III 241 0
33 * sig Sgr ** 18 55 15.92650 -26 17 48.2068 1.06 1.923 2.067     B2.5V 269 1
34 * bet Cep bC* 21 28 39.5968513 +70 33 38.574681 2.05 3.01 3.23 3.33 3.55 B0.5IIIs 725 0
35 * sig Phe Pu* 23 47 15.9964216632 -50 13 35.251982724   5.000 5.166     B3V 64 0

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