The magnetic structure of neutron stars and their surface-to-core temperature relation

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dc.creatorPotekhin, A. Y.
dc.creatorUrpin, V.
dc.creatorChabrier, G.
dc.date2005-08-19
dc.date2005-08-24
dc.date.accessioned2026-07-07T06:23:27Z
dc.date.available2026-07-07T06:23:27Z
dc.descriptionWe study the relation between the mean effective surface temperature T_s and the internal temperature T_b for magnetic neutron stars, assuming that the magnetic field near the surface has a presumably small-scale structure. The heavy-element (iron) and light-element (accreted) heat-blanketing envelopes are considered, and the results are compared with the case of a dipole magnetic field. We argue that the difference in the T_b(T_s)-relation for different magnetic configurations is always much smaller than a possible difference caused by variations of the chemical composition in the envelope.
dc.description5 pages, 2 figures. V2: a typo corrected. Accepted by A&A
dc.identifierhttps://arxiv.org/abs/astro-ph/0508415
dc.identifierhttp://arxiv.org/abs/astro-ph/0508415
dc.identifierAstron.Astrophys. 443 (2005) 1025-1028
dc.identifierdoi:10.1051/0004-6361:20053628
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/96241
dc.subjectAstrophysics
dc.titleThe magnetic structure of neutron stars and their surface-to-core temperature relation
dc.typetext

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