Table 4
Cluster models for estimating fly-by probabilities.
| Model name | Resembling | mcl (M⊙) | rh (pc) |  (M⊙) |
Nsolar | Reference |
|---|---|---|---|---|---|---|
| C1 | ONC | 2000 | 0.8 | 0.7 | 60 | [1] |
| C2 | Arches | 50000 | 0.2 | 1.6 | 3300 | [2] |
Notes. Here, mcl is the total cluster mass and rh is the half-mass radius. The mean stellar mass,
, and the approximate number of solar mass stars, Nsolar, were calculated based on the mass functions for the respective cluster. Model C2 resembles the “initial” Arches, not the contemporary Arches.
References. [1] Hillenbrand & Hartmann (1998); [2] Harfst et al. (2010).
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.