Table 7
Results of our Monte Carlo simulations of the detection of massive binaries with the sampling of the GIRAFFE-IFU campaign.
| m1 (M⊙) | I | II | III | IV | V |
| P ≤ 5 | 5 < P ≤ 10 | 10 < P ≤ 20 | 20 < P ≤ 50 | 50 < P ≤ 100 | |
| (%) | (%) | (%) | (%) | (%) | |
|
|
|||||
| 20 | 0.7 | 0.7 | 1.8 | 19.0 | 56.2 |
| 30 | 0.6 | 0.6 | 1.5 | 15.8 | 50.8 |
| 40 | 0.5 | 0.5 | 1.2 | 13.8 | 46.6 |
| 50 | 0.4 | 0.4 | 1.0 | 12.4 | 43.6 |
Notes. For a given range of orbital periods (expressed in days) and a given value of the primary mass, the table yields the fraction of systems (in % of the population of systems within this interval of periods) that would display ΔRV = maxRV(φi) − minRV(φi) < 20 km s-1, hence escape detection. The total numbers of simulated systems in each of the period intervals are 34198, 25802, 4786, 6315, and 4772 for the intervals I, II, III, IV, and V, respectively.
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.