Table 6.
Expected number of stars detected at 10 GHz within cylindrical beam of R = 0.5 pc, assuming a mass of 1 × 104 M⊙, a volume filling factor of 1, different ages and two different slopes a of the initial mass function.
| Age (Myr) | 2 | 3 | 4 | 5 |
|---|---|---|---|---|
| PARSEC | ||||
| a = 2.35 | 1.4 ± 1.2 (7.7 ± 2.6) | 4.7 ± 2.0 (6.4 ± 2.3) | 5.6 ± 2.7 (5.9 ± 2.7) | 3.4 ± 1.7 (5.6 ± 2.4) |
| a = 1.8 | 5.7 ± 2.1 (26.2 ± 4.8) | 17.6 ± 4.0 (22.6 ± 4.6) | 15.3 ± 3.7 (16.2 ± 3.9) | 7.9 ± 2.8 (12.8 ± 3.4) |
| MIST | ||||
| a = 2.35 | 2.5 ± 1.7 (8.1 ± 3.2) | 5.8 ± 2.4 (9.6 ± 3.5) | 3.3 ± 2.0 (3.5 ± 2.0) | 3.1 ± 1.8 (3.1 ± 1.8) |
| a = 1.8 | 9.6 ± 3.1 (27.1 ± 4.5) | 20.6 ± 4.2 (31.4 ± 5.3) | 10.1 ± 3.1 (10.5 ± 3.1) | 7.8 ± 2.9 (7.9 ± 2.8) |
Notes. The numbers in brackets correspond to the assumption of a volume filling factor of 0.1 for the stellar wind.
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.