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| author | Aaron LI <aly@aaronly.me> | 2018-01-16 09:23:52 +0800 |
|---|---|---|
| committer | Aaron LI <aly@aaronly.me> | 2018-01-16 09:23:52 +0800 |
| commit | 1200e50fd24451ed7b56d137a20106c18c0e0153 (patch) | |
| tree | ef73efe9315e8774556f3215ccf523b51c609b37 /fg21sim/configs | |
| parent | 8dcf5caa1e6b37d7717ea04167e96ebee3e9516a (diff) | |
| download | fg21sim-1200e50fd24451ed7b56d137a20106c18c0e0153.tar.bz2 | |
clusters: minor updates
Diffstat (limited to 'fg21sim/configs')
| -rw-r--r-- | fg21sim/configs/20-extragalactic.conf.spec | 2 |
1 files changed, 2 insertions, 0 deletions
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 |