A diffuse source.
This can be used for example to simulate the interstellar radiation field. This source emits inwards.
Parameters : | name : str, optional
peeloff : bool, optional
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Notes
Any additional arguments are are used to initialize attributes.
Attributes
luminosity | The bolometric luminosity of the source (ergs/s) |
temperature | The temperature of the source (K) |
spectrum | The spectrum of the source, specified either as an atpy.Table instance with 'nu' and 'fnu' columns, or as a (nu, fnu) tuple, where the frequency is given in Hz, and the flux is given as F_nu (units are unimportant since the normalization is set by the luminosity). |
map | The relative luminosity in each cell, given as a Numpy array or an AMRGridView instance |