Free Access
Table 2.
Estimated properties of stars of various effective temperatures, T⋆.
| T⋆ [K] | LMS [L⊙] | Radius [R⊙] | Q⋆ [s−1] |
|---|---|---|---|
| 10 000 | 46 | 2.3 | 7.8 × 1041 |
| 20 000 | 4200 | 5.4 | 2.7 × 1046 |
| 30 000 | 59 000 | 9.0 | 1.8 × 1048 |
| 40 000 | 4 × 105 | 13 | 2.0 × 1049 |
| 50 000 | 2 × 106 | 17 | 1.1 × 1050 |
Notes. LMS is the bolometric luminosity estimate from the temperature of a main sequence star, followed by the radius required to equate this to the bolometric intensity and finally the number of ionising photons per second.
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.