Comt: comptonisation model#
This is the model for Comptonisation of soft photons in a hot plasma, developed by Titarchuk (1994). See the XSPEC manual for more details. The code was substantially improved and brought to the SPEX standards.
Some modifications#
Titarchuk (1994) gives an analytical approximation for \(\beta(\tau\)) to the exact calculations as provided by Sunyaev & Titarchuk (1985) for \(0.1<\tau<10\). Their approximation has the proper asymptotic behaviour for small and large values of \(\tau\), but unfortunately has deviations up to 7 % over the \(0.1-10\) range for \(\tau\). The approximation by Titarchuk is given in their equations (27) and (28) by
We found an approximation that is better than 1 % using a slight modification of the above equations. We use these new approximations in our calculations:
Warning
For the physically valid range of parameters, consult the XSPEC manual; see also Hua & Titarchuk (1995), their Fig. 7.
The parameters of the model are:
norm : Normalisation \(A\) of the power law, in units of
\(10^{44}\) \(\mathrm{ph}\) \(\mathrm{s}^{-1}\)
\(\mathrm{keV}^{-1}\). Due to the way the model is calculated, this is not
the flux at 1 keV! Default value: 1.t0 : The temperature \(T\) of the seed photons in keV. Default
value: 1 keV.t1 : The plasma temperature \(T\) in keV. Default value: 100
keV.tau : The optical depth. Default value: 3.type : The type of geometry. Allowed values are 0 for a disk
(default) or 1 for a sphere. This is a frozen parameter (cannot be
fitted).Recommended citation: Titarchuk (1994)