The XSPEC cflow model: cooling flow.
xscflow The xscflow model is an additive model component.
The model is described at  . The results of this model depend on the cosmology settings set with set_xscosmo .
>>> create_model_component("xscflow", "mdl") >>> print(mdl)
Create a component of the xscflow model and display its default parameters. The output is:
mdl Param Type Value Min Max Units ----- ---- ----- --- --- ----- mdl.slope thawed 0 -5 5 mdl.lowT thawed 0.1 0.0808 79.9 keV mdl.highT thawed 4 0.0808 79.9 keV mdl.Abundanc thawed 1 0 5 mdl.redshift frozen 0.1 1e-10 10 mdl.norm thawed 1 0 1e+24
The attributes for this object are:
The power-law index of the emissivity function.
The minimum temperature, in keV.
The maxmimum temperature, in keV.
The abundance relative to Solar, as set by set_xsabund .
The redshift of the plasma.
The mass accretion rate (solar mass per year).
-  https://heasarc.gsfc.nasa.gov/xanadu/xspec/manual/XSmodelCflow.html
CIAO 4.12 comes with support for version 12.10.1n of the XSPEC models. This can be checked with the following:
% python -c 'from sherpa.astro import xspec; print(xspec.get_xsversion())' 12.10.1n
See the bugs pages on the Sherpa website for an up-to-date listing of known bugs.