Stellar parameters adopted for G 29-38 and GD 133.
|Star||MWD [M⊙]||Teff [K]||log MH/MWD||log Mcvz/MWD|
|G 29-38||0.85||11 820 ± 100||10-4||−13.95|
|GD 133||0.63||12 400 ± 100||3.16 × 10-5||−16.19|
Notes. For G 29-38, the mass and the effective temperature are the values derived from spectroscopy (Xu et al. 2014). For GD 133, the values are derived from the asteroseismology analysis of Fu et al. (2016). They are in good agreement with the values given by spectroscopy (Xu et al. 2014). The hydrogen mass fractions are from asteroseismology: Chen & Li (2013) for G 29-38, and Fu et al. (2016) for GD 133.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.