Table 1
Summary of stellar parameters used in this paper.
| M⋆ ∕M⊙ | Rc ∕R⊙ | log(L∕L⊙) | vesc (km s−1) |
|---|---|---|---|
| 10 | 1 | 5.416 | 1950 |
Notes. Here we set our standard stellar parameters such that they roughly represent the average value of the mass-to-radius ratio of the observationally inferred WRstellar population from Hamann et al. (2019) and Sander et al. (2019). The luminosity is then set such that the resulting Γe = 0.40, also corresponding to the observationally inferred average (Hamann et al. 2019; Sander et al. 2019).
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.