diff options
| -rw-r--r-- | fg21sim/extragalactic/clusters/halo.py | 2 | ||||
| -rw-r--r-- | fg21sim/extragalactic/clusters/helper.py | 6 |
2 files changed, 4 insertions, 4 deletions
diff --git a/fg21sim/extragalactic/clusters/halo.py b/fg21sim/extragalactic/clusters/halo.py index beaff9e..ab59db9 100644 --- a/fg21sim/extragalactic/clusters/halo.py +++ b/fg21sim/extragalactic/clusters/halo.py @@ -232,7 +232,7 @@ class RadioHalo: Unit: [keV] """ mass = self.M_main + self.M_sub - kT = helper.mass_to_kT(mass, z=self.z_merger) + kT = helper.kT_cluster(mass, z=self.z_merger) return kT @property diff --git a/fg21sim/extragalactic/clusters/helper.py b/fg21sim/extragalactic/clusters/helper.py index daf806b..e43d7f4 100644 --- a/fg21sim/extragalactic/clusters/helper.py +++ b/fg21sim/extragalactic/clusters/helper.py @@ -241,10 +241,10 @@ def density_energy_thermal(mass, z=0.0): ------- e_th : float Energy density of the ICM - Unit: [erg cm^-3] + Unit: [erg/cm^3] """ - n_th = density_number_thermal(mass, z) # [cm^-3] - kT = mass_to_kT(mass, z) * AUC.keV2erg # [erg] + n_th = density_number_thermal(mass=mass, z=z) # [cm^-3] + kT = kT_cluster(mass, z) * AUC.keV2erg # [erg] e_th = (3.0/2) * kT * n_th return e_th |