Table 1
Stellar parameters for B0-type star (Harmanec 1988, see also Kurfürst et al. 2014) and for typical Pop III star (e.g., Marigo et al. 2001) used in the models.
| B0-type star: | ||||
|---|---|---|---|---|
| M⋆(M⊙) | R⋆(R⊙) | Req(R⊙) | ⟨Teff⟩(K) | Z |
| 14.5 | 5.8 | 8.7 | 30 000 | 0.005 |
| Pop III star: | ||||
| M⋆(M⊙) | R⋆(R⊙) | Req(R⊙) | ⟨Teff⟩(K) | Z |
| 40 | 30 | 45 | 25 000 | 0 |
Notes. A selected metallicity Z for B0-type star may roughly correspond to an average of Magellanic Clouds (e.g., Rivinius et al. 2013) while we assume for simplicity Z = 0 in the models of dense disks, corresponding to Pop III stars.
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.