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| author | Aaron LI <aly@aaronly.me> | 2017-10-18 16:14:59 +0800 |
|---|---|---|
| committer | Aaron LI <aly@aaronly.me> | 2017-10-18 16:16:18 +0800 |
| commit | 375198fb380933ea1b00f2e42401550ae20da76d (patch) | |
| tree | 966fa37fd3e1b5f5f32c0ad30f927524f7d40f39 /fg21sim/extragalactic/clusters/mergertree.py | |
| parent | 3dadf7b53f28af00f3170a10629c91e8d2888e0e (diff) | |
| download | fg21sim-375198fb380933ea1b00f2e42401550ae20da76d.tar.bz2 | |
clusters: Update radio halo radius estimation
The simulated radio halo is assumed to have a radius of the falling
sub-cluster; while previously it is assumed to be 1/4 of the virial radius of
the merged cluster.
The new estimation can agree better with the currently observed radio halos,
which generally have a angular diameter size of ~2-7 [arcmin].
Diffstat (limited to 'fg21sim/extragalactic/clusters/mergertree.py')
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