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AGN.autogen
An advanced option - this is a low frequency cutoff for an AGN power law spectrum. It prevents the powerlaw being applied to low frequencies and giving an odd SED.
Type: Double
Unit: Hz
Values: Greater than 0
Parent(s):
- :ref:`BH.radiation`:
True
File: setup_star_bh.c
The exponent alpha in a power law SED applied to an AGN central source of the form L_nu=K nu**alpha
Type: Double
Values: Any - but sign is not assumed, so for negative index use a negative value
Parent(s):
- :ref:`BH.radiation`:
True
File: setup_star_bh.c
The frequency exponent alpha in bremstrahlung SED of the form L_nu=nu**alpha exp(-hnu/kT)
Type: Double
Values: Any - sign is not assumed so use negative if you want negative
Parent(s):
- :ref:`BH.rad_type_to_make_wind`: brems
File: setup_star_bh.c
The temperature T in bremstrahlung SED of the form L_nu=nu**alpha exp(-hnu/kT)
Type: Double
Unit: K
Values: Greater than 0
Parent(s):
- :ref:`BH.rad_type_to_make_wind`: brems
File: setup_star_bh.c
Generates the AGN/BH source from two points, located symmetrically above the axes of the central object.
Type: Double
Unit: :ref:`Central_object.radius`
Values: Greater than 0
Parent(s):
- :ref:`BH.geometry_for_pl_source`: lamp_post
File: setup_star_bh.c