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Query : 2002A&A...389..162N |
2002A&A...389..162N - Astronomy and Astrophysics, volume 389, 162-179 (2002/7-1)
The mass-loss rates of Wolf-Rayet stars explained by optically thick radiation driven wind models.
NUGIS T. and LAMERS H.J.G.L.M.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): stars: atmospheres - stars: mass-loss - stars: emission-lines - stars: evolution - stars: Wolf-Rayet
Simbad objects: 9
Number of rows : 9 |
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 | HD 6327 | WR* | 01 05 23.0143603 | +60 25 18.965197 | 11.49 | 11.33 | WN2-w | 120 | 0 | |||
2 | HD 92740 | WR* | 10 41 17.5158425712 | -59 40 36.895992960 | 5.68 | 6.50 | 6.42 | 7.38 | WN7h+O9III-V | 411 | 0 | |
3 | HD 97152 | WR* | 11 10 04.0797150120 | -60 58 44.963276664 | 7.47 | 8.03 | 8.07 | 8.91 | WC7+O7V | 183 | 0 | |
4 | HD 164270 | WR* | 18 01 43.1453595672 | -32 42 55.161329040 | 8.52 | 8.97 | 8.74 | 9.51 | WC9d+? | 225 | 0 | |
5 | EM* AS 268 | WR* | 18 02 23.4574037952 | -23 34 37.491692196 | 14.38 | 12.31 | 11.43 | WN9h | 101 | 0 | ||
6 | HD 165763 | WR* | 18 08 28.4692108104 | -21 15 11.183076540 | 7.16 | 7.54 | 7.82 | 8.55 | WC6 | 281 | 0 | |
7 | HD 192163 | WR* | 20 12 06.5418877464 | +38 21 17.784181008 | 7.12 | 7.49 | 7.50 | WN6(h)-s | 544 | 0 | ||
8 | HD 193576 | WR* | 20 19 32.4229160448 | +38 43 53.959035756 | 8.15 | 8.53 | 8.00 | WN5+O6II-V | 704 | 0 | ||
9 | HD 214419 | WR* | 22 36 53.9548302648 | +56 54 20.989190232 | 8.68 | 9.376 | 8.996 | 8.962 | WN6o+O9Ib/II | 376 | 1 |
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