diff options
Diffstat (limited to 'fg21sim/extragalactic/clusters')
| -rw-r--r-- | fg21sim/extragalactic/clusters/helper.py | 31 | 
1 files changed, 0 insertions, 31 deletions
diff --git a/fg21sim/extragalactic/clusters/helper.py b/fg21sim/extragalactic/clusters/helper.py index 3f7a964..9c900be 100644 --- a/fg21sim/extragalactic/clusters/helper.py +++ b/fg21sim/extragalactic/clusters/helper.py @@ -473,37 +473,6 @@ def velocity_impact(M_main, M_sub, z=0.0):      return vi / AUC.km2cm  # [km/s] -def time_crossing(M_main, M_sub, z=0.0): -    """ -    Estimate the crossing time of the sub cluster during a merger. - -    NOTE: The crossing time is estimated to be τ ~ R_vir / v_impact. - -    Parameters -    ---------- -    M_main, M_sub : float -        Total (virial) masses of the main and sub clusters -        Unit: [Msun] -    z : float, optional -        Redshift - -    Returns -    ------- -    time : float -        Crossing time -        Unit: [Gyr] - -    References -    ---------- -    Ref.[cassano2005],Sec.(4.1) -    """ -    R_vir = radius_virial(M_main, z)  # [kpc] -    vi = velocity_impact(M_main, M_sub, z)  # [km/s] -    uconv = AUC.kpc2km * AUC.s2Gyr  # [s kpc/km] => [Gyr] -    time = uconv * R_vir / vi  # [Gyr] -    return time - -  def draw_halo(radius, nr=2.0, felong=None, rotation=None):      """      Draw the template image of one halo, which is used to simulate  | 
