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| Query : 1991AGAb....6...48H |
1991AGAb....6...48H - Astron. Gesellschaft Abstract Ser., 6, 48-48 (1991)
A two-component disk-model for the fine-structure of Balmer emission lines in the spectra of Be stars.
HUMMEL W. and DACHS J.
Journal keyword(s):
Simbad objects: 3
| Number of rows : 3 |
| 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 | * alf Col | Be* | 05 39 38.9410319 | -34 04 26.794991 | 2.10 | 2.53 | 2.65 | 2.65 | 2.74 | B9Ve | 251 | 0 |
| 2 | * ups01 Pup | Be* | 07 18 18.3935775563 | -36 44 02.228526718 | 3.78 | 4.57 | 4.67 | 4.57 | 4.62 | B2V+B3IVne | 164 | 0 |
| 3 | HD 110432 | HXB | 12 42 50.2663572384 | -63 03 31.052981412 | 4.79 | 5.58 | 5.31 | B0.5IVpe | 334 | 0 |
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