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authorAaron LI <aly@aaronly.me>2018-10-25 11:56:59 +0800
committerAaron LI <aly@aaronly.me>2018-10-25 11:56:59 +0800
commita97128f666cbc61e1fd255a339001a9ad490c006 (patch)
tree33f7260334d5aaa4a295bab2b99533fa9fa9d08b /fg21sim/extragalactic/clusters/helper.py
parent087822f918a0d6a814da064281305c8fde31b8fa (diff)
downloadfg21sim-a97128f666cbc61e1fd255a339001a9ad490c006.tar.bz2
clusters/halo: Improve descriptions and comments
Diffstat (limited to 'fg21sim/extragalactic/clusters/helper.py')
-rw-r--r--fg21sim/extragalactic/clusters/helper.py2
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)