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authorAaron LI <aly@aaronly.me>2018-01-16 09:23:52 +0800
committerAaron LI <aly@aaronly.me>2018-01-16 09:23:52 +0800
commit1200e50fd24451ed7b56d137a20106c18c0e0153 (patch)
treeef73efe9315e8774556f3215ccf523b51c609b37 /fg21sim/configs/20-extragalactic.conf.spec
parent8dcf5caa1e6b37d7717ea04167e96ebee3e9516a (diff)
downloadfg21sim-1200e50fd24451ed7b56d137a20106c18c0e0153.tar.bz2
clusters: minor updates
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-rw-r--r--fg21sim/configs/20-extragalactic.conf.spec2
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diff --git a/fg21sim/configs/20-extragalactic.conf.spec b/fg21sim/configs/20-extragalactic.conf.spec
index cb11bd8..7de9eb1 100644
--- a/fg21sim/configs/20-extragalactic.conf.spec
+++ b/fg21sim/configs/20-extragalactic.conf.spec
@@ -132,6 +132,8 @@
# The fraction of the magnetic field energy density w.r.t. the ICM
# thermal energy density, which is used to determine the mean magnetic
# field strength within the ICM and is also assumed to be uniform.
+ # * ~< 0.4% (Ref: Pfrommer & Ensslin 2004, MNRAS)
+ # * ~0.3%-1% (Ref: Bohringer et al. 2016, A&A)
eta_b = float(default=0.001, min=1e-5, max=0.1)
# The temperature of the outer gas surrounding the cluster. Accretion