Equation of state and opacities for hydrogen atmospheres of strongly magnetized cooling neutron stars

Details Equation of state and opacities for hydrogen atmospheres of strongly magnetized cooling neutron stars Equation of state and opacities for hydrogen atmospheres of strongly magnetized cooling neutron stars

1998-03-05

arxiv.org/abs/astro-ph/9803046v2

Astronomy and Astrophysics

Astrophysics

4 pages, 2 embedded figures, LaTeX using epsf.sty, neu.sty, and tron.sty (included). PostScript version also available at ht

Scientific paper

We study partially ionized hydrogen plasma at temperatures T =
10^{5.5}-10^{6.5} K and magnetic fields B = 10^{12}-10^{13} G, typical of
photospheres of isolated neutron stars. We construct an analytic model of the
plasma free energy and derive a generalized Saha equation which is used to
obtain the opacities.

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