XSvnpshock¶
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class
sherpa.astro.xspec.XSvnpshock(name='vnpshock')[source]¶ Bases:
sherpa.astro.xspec.XSAdditiveModelThe XSPEC vnpshock model: shocked plasma, plane parallel, separate ion, electron temperatures.
The model is described at [1]. The
set_xsxsetandget_xsxsetfunctions are used to set and query the XSPEC XSET parameters, in particular the keyword “NEIVERS”.-
kT_a¶ The mean shock temperature, in keV.
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kT_b¶ The electron temperature immediately behind the shock front, in keV. See [1] for a discussion of the behavior of kT_a and kT_b.
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H¶ The H abundance: it should be set to 0 to switch on and 1 to switch off the free-free continuum.
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He, C, N, O, Ne, Mg, Si, S, Ar, Ca, Fe, Ni The abundance of the element, with respect to Solar.
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Tau_l¶ The lower limit on the ionization timescale in s/cm^3.
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Tau_u¶ The upper limit on the ionization timescale in s/cm^3.
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redshift¶ The redshift of the source.
See also
References
[1] (1, 2, 3) https://heasarc.gsfc.nasa.gov/xanadu/xspec/manual/XSmodelNpshock.html Attributes Summary
thawedparhardmaxesthawedparhardminsthawedparmaxesthawedparminsthawedparsversion_enabledMethods Summary
apply(outer, \*otherargs, \*\*otherkwargs)calc(pars, xlo, \*args, \*\*kwargs)get_center()guess(dep, \*args, \*\*kwargs)reset()set_center(\*args, \*\*kwargs)startup()teardown()Attributes Documentation
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thawedparhardmaxes¶
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thawedparhardmins¶
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thawedparmaxes¶
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thawedparmins¶
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thawedpars¶
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version_enabled= True¶
Methods Documentation
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apply(outer, *otherargs, **otherkwargs)¶
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calc(pars, xlo, *args, **kwargs)¶
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get_center()¶
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guess(dep, *args, **kwargs)¶
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reset()¶
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set_center(*args, **kwargs)¶
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startup()¶
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teardown()¶
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