Table 1
Studied sample of Be stars and their apparent fundamental parameters.
| HD |
|
|
log Lapp/L⊙ | E(B − V) ± σE | (Vsini)app | Notes |
| ± σlog g | ± σlog L | ± σVsini | ||||
| K | dex | dex | mag | km s-1 | ||
|
|
||||||
| 144 | 12 180 ± 170 | 3.80 ± 0.10 | 2.964 ± 0.026 | 0.08 ± 0.03 | 125 ± 6 | 1, f |
| 4180 | 15 520 ± 360 | 3.54 ± 0.31 | 3.426 ± 0.037 | 0.11 ± 0.02 | 195 ± 10 | 1, f |
| 5394 | 35 210 ± 2130 | 4.18 ± 0.31 | 5.190 ± 0.055 | 0.13 ± 0.07 | 432 ± 34 | 1, f |
| ... | ... | ... | ... | ... | ... | ... |
| 330 950 | 29 870 ± 3390 | 4.45 ± 0.38 | 2.578 ± 0.120 | 0.69 ± 0.13 | 60 ± 4 | 2, 4, d |
Notes. 1: stars studied in Chauville et al. (2001), Frémat et al. (2005), Zorec et al. (2005); 2: stars studied in Levenhagen & Leister (2006); 3: stars studied in Frémat et al. (2006); 4: stars with new BCD observations (Cochetti 2014); f: stars with integrated fluxes; and d: stars with spectroscopic distances. The complete version of this table is available at the CDS.
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