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author | Aaron LI <aly@aaronly.me> | 2018-10-25 11:56:59 +0800 |
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committer | Aaron LI <aly@aaronly.me> | 2018-10-25 11:56:59 +0800 |
commit | a97128f666cbc61e1fd255a339001a9ad490c006 (patch) | |
tree | 33f7260334d5aaa4a295bab2b99533fa9fa9d08b /fg21sim/extragalactic/clusters/helper.py | |
parent | 087822f918a0d6a814da064281305c8fde31b8fa (diff) | |
download | fg21sim-a97128f666cbc61e1fd255a339001a9ad490c006.tar.bz2 |
clusters/halo: Improve descriptions and comments
Diffstat (limited to 'fg21sim/extragalactic/clusters/helper.py')
-rw-r--r-- | fg21sim/extragalactic/clusters/helper.py | 2 |
1 files changed, 1 insertions, 1 deletions
diff --git a/fg21sim/extragalactic/clusters/helper.py b/fg21sim/extragalactic/clusters/helper.py index 5fd25a9..b58dc87 100644 --- a/fg21sim/extragalactic/clusters/helper.py +++ b/fg21sim/extragalactic/clusters/helper.py @@ -97,7 +97,7 @@ def radius_halo(mass, z=0.0, configs=CONFIGS): ---- The halo radius is estimated to be the same as the turbulence injection scale, i.e.: - R_halo ≅ L ≅ R_vir / 3 + R_halo ≅ L_turb ≅ R_vir / 3 where R_vir the virial radius of the merged (observed) cluster. Reference: [vazza2011],Sec.(3.6) |