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author | Aaron LI <aly@aaronly.me> | 2017-10-22 15:17:07 +0800 |
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committer | Aaron LI <aly@aaronly.me> | 2017-10-22 15:17:07 +0800 |
commit | a42a613f3a1328ca0582bef19e024868fa3a3ad5 (patch) | |
tree | 9110f264c422ef850bac3640ab50e331ec292ca6 /fg21sim/extragalactic/clusters/helper.py | |
parent | 0ddacb9b2dd050e84f889662f09bf686cfae3d33 (diff) | |
download | fg21sim-a42a613f3a1328ca0582bef19e024868fa3a3ad5.tar.bz2 |
clusters/halo: Add option "kT_out" to tune cluster temperature
Diffstat (limited to 'fg21sim/extragalactic/clusters/helper.py')
-rw-r--r-- | fg21sim/extragalactic/clusters/helper.py | 8 |
1 files changed, 6 insertions, 2 deletions
diff --git a/fg21sim/extragalactic/clusters/helper.py b/fg21sim/extragalactic/clusters/helper.py index d77c63e..86662e1 100644 --- a/fg21sim/extragalactic/clusters/helper.py +++ b/fg21sim/extragalactic/clusters/helper.py @@ -153,7 +153,9 @@ def kT_cluster(mass, z=0.0, radius=None): the cluster (near the virial radius) which can heat the gas, therefore the ICM has a higher temperature than the virial temperature, which can be estimated as: - T_icm = T_vir + 1.5*T_1 ~ T_vir + 0.8 [keV] + kT_icm ~ kT_vir + 1.5 * kT_out + where kT_out the temperature of the outer gas surround the cluster, + which may be ~0.5-1.0 keV. Reference: Ref.[fujita2003],Eq.(49) @@ -163,8 +165,10 @@ def kT_cluster(mass, z=0.0, radius=None): The temperature of the cluster ICM. Unit: [keV] """ + key = "extragalactic/clusters/kT_out" + kT_out = CONFIGS.getn(key) kT_vir = kT_virial(mass=mass, z=z, radius=radius) - kT_icm = kT_vir + 0.8 + kT_icm = kT_vir + 1.5*kT_out return kT_icm |