Table 7.
Masses of the bodies in γ Cep found in the literature.
| Source | Method | MA | Method | MB | Method | MAb | MAb sin iAb |
|---|---|---|---|---|---|---|---|
| MA | (M⊙) | MB | (M⊙) | MAb | (MJup) | (MJup) | |
| Fuhrmann (2004) | Spectroscopy | 1.59 | – | – | – | – | – |
| Hatzes et al. (2003) | Fuhrmann (2004) | 1.59 ± 0.12 | – | – | Derived | – | 1.7 ± 0.4 |
| Torres (2007) | Spec. & phot. | 1.18 ± 0.11 | Derived | 0.362 ± 0.022 | – | – | 1.43 ± 0.13 |
| Neuhäuser et al. (2007) | Dynamical | 1.40 ± 0.12 | Dynamical | 0.409 ± 0.018 | – | – | 1.60 ± 0.13 |
| Mortier et al. (2013, Table 5) | Spectroscopy | 1.26 ± 0.14 | – | – | – | – | – |
| Stello et al. (2017) | Asteroseismology | 1.32 ± 0.20 | – | – | – | – | – |
| Baines et al. (2018) | Interfero. (model) | 1.41 ± 0.08 | – | – | – | – | – |
| Malla et al. (2020) | Asteroseismology | 1.32 ± 0.12 | – | – | – | – | – |
| This work | Asteroseismology |
 |
Derived |
 |
Derived |
 |
1.41 ± 0.08 |
Notes. Here we only report on values explicitly reported in any of the given papers. The method denotes the approach used to derive the quantity, the masses of MB and MAb this are typically derived from the mass function, with the exception of dynamically determined masses. Hatzes et al. (2003) have used the mass estimate from Fuhrmann (2004), who states that typical errors for the mass are less than 10% for the stars in that study.
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