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| Query : 1983A&A...124..283B |
1983A&A...124..283B - Astronomy and Astrophysics, volume 124283-286 (1983)
Can shell phases of Be stars be predicted on the basis of rapid spectroscopic micro-variability ?
BAADE D.
Journal keyword(s):
Simbad objects: 5
| Number of rows : 5 |
| 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 | * zet Tau | Be* | 05 37 38.6854231 | +21 08 33.158804 | 2.22 | 2.84 | 3.03 | 3.06 | 3.15 | B1IVe_shell | 751 | 0 |
| 2 | * 27 CMa | Be* | 07 14 15.2117197408 | -26 21 09.028965559 | 3.76 | 4.45 | 4.65 | 4.64 | 4.73 | B4Ve_sh | 240 | 0 |
| 3 | * eta Cen | Be* | 14 35 30.4241610 | -42 09 28.170782 | 1.30 | 2.12 | 2.31 | 2.41 | 2.59 | B2Ve | 361 | 1 |
| 4 | * 48 Lib | Be* | 15 58 11.3682502453 | -14 16 45.681109093 | 4.61 | 4.77 | 4.87 | 4.91 | 4.96 | B5IIIp_sh | 446 | 0 |
| 5 | * omi And | Be* | 23 01 55.2649954408 | +42 19 33.655865640 | 3.00 | 3.53 | 3.62 | 3.61 | 3.69 | B6IV/V_sh | 437 | 0 |
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