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Table 5
Mass and radius from the literature.
| Star | M p | M s | R p | R s | Reference |
| [M⊙] | [M⊙] | [R⊙] | [R⊙] | ||
|
|
|||||
| V478 Cyg | 15.3 ± 0.8 | 14.6 ± 0.8 | 7.6 ± 0.1 | 8.5 ± 0.1 | this work |
| 16.6 ± 0.9 | 16.3 ± 0.9 | 7.43 ± 0.12 | 7.43 ± 0.12 | Popper & Hill (1991) | |
| Y Cyg | 16.9 ± 0.5 | 16.0 ± 0.5 | 5.9 ± 0.1 | 5.1 ± 0.1 | this work |
| 16.8 ± 0.5 | 17.7 ± 0.4 | – | – | Burkholder et al. (1997) | |
| 17.72 ± 0.35 | 17.73 ± 0.30 | 5.785 ± 0.091 | 5.816 ± 0.063 | Harmanec et al. (2014) | |
| 17.57 ± 0.27 | 17.04 ± 0.26 | 5.93 ± 0.07 | 5.78 ± 0.07 | Simon et al. (1994) | |
| V382 Cyg | 26.1 ± 0.4 | 19.0 ± 0.3 | 9.4 ± 0.2 | 8.7 ± 0.2 | this work |
| 32.6 ± 1.8 | 22.9 ± 1.3 | 8.8 ± 0.6 | 7.4 ± 0.6 | Popper & Hill (1991) | |
| 29.7 ± 1.1 | 20.3 ± 0.9 | – | – | Burkholder et al. (1997) | |
| 26.0 ± 0.7 | 19.3 ± 0.4 | 9.6 ± 0.1 | 8.4 ± 0.1 | Harries et al. (1997) | |
| XZ Cep | 18.7 ± 1.3 | 9.3 ± 0.5 | 14.2 ± 0.1 | 14.2 ± 0.1 | this work |
| 15.8 ± 0.4 | 6.4 ± 0.3 | 7.0 ± 0.2 | 140.5 ± 0.2 | Harries et al. (1997) | |
| AH Cep | 14.3 ± 1.0 | 12.6 ± 0.9 | 5.6 ± 0.1 | 4.7 ± 0.1 | this work |
16.2 |
13.3 |
– | – | Burkholder et al. (1997) | |
| 18.1 ± 0.9 | 15.9 ± 0.8 | 6.7 ± 0.2 | 6.2 ± 0.2 | Bell et al. (1986) | |
| DH Cep1 | 38.4 ± 2.5 | 33.4 ± 2.2 | – | – | this work |
34.4 |
29.8 |
– | – | Burkholder et al. (1997) | |
| 32.7 ± 1.7 | 29.6 ± 1.6 | – | – | Hilditch et al. (1996) | |
Notes. 1- For DH Cep, we assume an inclination of 47o ± 1, according to Sturm & Simon (1994), to obtain the dynamical masses.
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