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| author | Aaron LI <aly@aaronly.me> | 2019-01-26 22:13:49 +0800 |
|---|---|---|
| committer | Aaron LI <aly@aaronly.me> | 2019-01-26 22:13:49 +0800 |
| commit | c9f0dbf07992a67591881e5a092b5366b2611939 (patch) | |
| tree | 3f4b13b7ae1d49b85a39fb847879ca3b2c6bba9c | |
| parent | 55128a7f3bf5b01f5480b2e29bd2021353cb9991 (diff) | |
| download | fg21sim-c9f0dbf07992a67591881e5a092b5366b2611939.tar.bz2 | |
clusters/main: Adjust against halo radius
| -rw-r--r-- | fg21sim/extragalactic/clusters/main.py | 7 |
1 files changed, 3 insertions, 4 deletions
diff --git a/fg21sim/extragalactic/clusters/main.py b/fg21sim/extragalactic/clusters/main.py index 20069bb..a4b63fa 100644 --- a/fg21sim/extragalactic/clusters/main.py +++ b/fg21sim/extragalactic/clusters/main.py @@ -1,5 +1,5 @@ # Copyright (c) 2017-2019 Weitian LI <wt@liwt.net> -# MIT license +# MIT License """ Simulate the diffuse radio emissions from galaxy clusters. @@ -293,13 +293,12 @@ class GalaxyClusters: z_merger=clinfo["merger_z"], merger_num=merger_num, configs=self.configs) - radius = halo.calc_radius() # [kpc] - theta = radius / (clinfo["DA"]*1e3) * AUC.rad2arcsec # [arcsec] + theta = halo.radius / (clinfo["DA"]*1e3) * AUC.rad2arcsec # [arcsec] n_e = halo.calc_electron_spectrum() haloinfo = OrderedDict( **clinfo, - Rhalo=radius, # [kpc] + Rhalo=halo.radius, # [kpc] Rhalo_angular=theta, # [arcsec] n_e=n_e, # [cm^-3] gamma=halo.gamma, # Lorentz factors |