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

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dc.creatorPotekhin, A. Y.
dc.creatorShibanov, Yu. A.
dc.creatorVentura, J.
dc.date1998-03-05
dc.date1999-03-09
dc.date.accessioned2026-07-07T02:26:16Z
dc.date.available2026-07-07T02:26:16Z
dc.descriptionWe 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.
dc.description4 pages, 2 embedded figures, LaTeX using epsf.sty, neu.sty, and tron.sty (included). PostScript version also available at http://www.ioffe.rssi.ru/dtastrop.html Published in "Neutron Stars and Pulsars," eds. N. Shibazaki et al. (Universal Academy Press, Tokyo, 1998) p. 161
dc.identifierhttps://arxiv.org/abs/astro-ph/9803046
dc.identifierhttp://arxiv.org/abs/astro-ph/9803046
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12207
dc.subjectAstrophysics
dc.subjectPlasma Physics
dc.titleEquation of state and opacities for hydrogen atmospheres of strongly magnetized cooling neutron stars
dc.typetext

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