Table 2
Observed parameters from Josselin & Plez (2007) with the addition of Antares as observed by Ohnaka et al. (2013, 2017), including vturb as required by theory to recover the mass-loss rate keeping all other parameters fixed.
Number | Name | Mass | Teff | Radius | Ṁgas (a) | ||
---|---|---|---|---|---|---|---|
(M⊙) | (K) | (R⊙) | (10−7 M⊙ yr−1) | (km s−1) | |||
1 | α Ori | 15 | 3780 | 589 | 5.0 | 19 | 17 |
2 | V466 Cas | 12 | 3780 | 331 | 0.5 | 12 | 19 |
3 | AD Per | 12 | 3720 | 457 | 2.0 | 21 | 17 |
4 | FZ Per | 12 | 3920 | 324 | 1.75 | 16 | 20 |
5 | BD+243902 | 15 | 4240 | 427 | 7.25 | 23 | 21 |
6 | BI Cyg | 20 | 3720 | 851 | 10.25 | 23 | 16 |
7 | BC Cyg | 20 | 3570 | 1230 | 8.0 | 22 | 13 |
8 | RW Cyg | 20 | 3920 | 676 | 8.25 | 20 | 19 |
9 | SW Cep | 9 | 3570 | 234 | 11.5 | 24 | 23 |
10 | μ Cep | 25 | 3750 | 1259 | 3.75 | 23 | 14 |
11 | ST Cep | 9 | 4200 | 174 | 6.25 | 23 | 26 |
12 | TZ Cas | 15 | 3670 | 646 | 9.5 | 17 | 17 |
13 | Antares | 12.7(1) | 3660(1) | 680(1) | 20.0(2) | 20(3) | 15 |
Notes. (a) A constant gas to dust mass ratio 250 has beenassumed to convert Ṁdust as compiled by Josselin & Plez (2007) to Ṁgas.
References.(1)Ohnaka et al. (2013), (2)Braun et al. (2012), (3)Ohnaka et al. (2017).
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