Black Hole SourcesΒΆ
Black hole sources currently have a wider array of potential behaviors than stellar sources. For example, their spectra can be quite a bit more complicated. ares supports several standard SEDs for BHs:
- Power-law (see
source_alpha
parameter to set slope) - Absorbed power-law (see
source_logN
to set absorbing column) - The multi-color disk spectrum
BHs are also normalized differently.