pyCloudy
0.9.6
manage Cloudy photoionization code
|
Classes | |
class | CST |
Functions | |
def | flux_convert (x, y, x_unit, y_unit_in, y_unit_out) |
def | planck |
def | atomic_mass (elem) |
Variables | |
dictionary | ATOMIC_MASS = {} |
dictionary | abund_Asplund_2009 |
dictionary | abund_Lodder_2003 |
dictionary | depletion_cloudy_13 = {} |
dictionary | depletion_dopita_2013 = {} |
dictionary | depletion_jenkins_2009 = {} |
dictionary | depletion_jenkins_2009l = {} |
def pyCloudy.utils.physics.atomic_mass | ( | elem | ) |
def pyCloudy.utils.physics.flux_convert | ( | x, | |
y, | |||
x_unit, | |||
y_unit_in, | |||
y_unit_out | |||
) |
def pyCloudy.utils.physics.planck | ( | T, | |
x = None , |
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x_min = None , |
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x_max = None , |
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n_steps = 1000 , |
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x_log = True , |
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x_unit = 'Angstrom' , |
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y_unit = 'erg/s/cm2/A' |
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) |
dictionary abund_Asplund_2009 |
dictionary abund_Lodder_2003 |
dictionary ATOMIC_MASS = {} |
dictionary depletion_cloudy_13 = {} |
dictionary depletion_dopita_2013 = {} |
dictionary depletion_jenkins_2009 = {} |
dictionary depletion_jenkins_2009l = {} |