Surface Temperature of Magnetized Neutron Stars

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dc.creatorPage, Dany
dc.creatorSarmiento, A.
dc.date1996-01-31
dc.date.accessioned2026-07-07T02:20:50Z
dc.date.available2026-07-07T02:20:50Z
dc.descriptionWe show that the expected inhomogeneous temperature distribution induced at the surface of a neutron star by the anisotropy of heat transport in the magnetized envelope allows us to understand quite well the observed pulse profiles of the four nearby pulsars for which surface thermal emission has been detected. However, due to gravitational lensing, dipolar magnetic fields are not adequate and the observed high pulsed fractions force us to include a quadrupolar component.
dc.description2 pages Latex with 1 figure and 1 heading in postscript. Style file: xray-wuerzburg-95.sty
dc.identifierhttps://arxiv.org/abs/astro-ph/9601175
dc.identifierhttp://arxiv.org/abs/astro-ph/9601175
dc.identifier`Roentgenstrahlung from the Universe', MPE Report 263 (1996) 171
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10346
dc.subjectAstrophysics
dc.titleSurface Temperature of Magnetized Neutron Stars
dc.typetext

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