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arXiv.org e-Print Archive
Preprint . 1996
Data sources: arXiv.org e-Print Archive
https://dx.doi.org/10.48550/ar...
Article . 1996
License: arXiv Non-Exclusive Distribution
Data sources: Datacite
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Surface Temperature of Magnetized Neutron Stars

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 01 Jan 1996Embargo end date: 01 Jan 1996Publisher:arXiv
Authors: Page, Dany; Sarmiento, A.;

doi: 10.48550/arxiv.astro-ph/9601175

arXiv: http://arxiv.org/abs/astro-ph/9601175

Surface Temperature of Magnetized Neutron Stars

Abstract

We 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.

2 pages Latex with 1 figure and 1 heading in postscript. Style file: xray-wuerzburg-95.sty

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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