Volume 443, Number 3, December I 2005
|Page(s)||1025 - 1028|
|Section||Stellar structure and evolution|
|Published online||15 November 2005|
The magnetic structure of neutron stars and their surface-to-core temperature relation
École Normale Supérieure de Lyon (CRAL, CNRS UMR 5574), 46 allée d'Italie, 69364 Lyon Cedex 07, France
2 Ioffe Physico-Technical Institute, Politekhnicheskaya 26, 194021 St. Petersburg, Russia e-mail: firstname.lastname@example.org
3 Isaac Newton Institute of Chile, St. Petersburg Branch, Russia
Accepted: 9 August 2005
We study the relation between the mean effective surface temperature and the internal temperature for magnetic neutron stars, assuming that the magnetic field near the surface has a 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 -relation for different magnetic configurations is always much smaller than the possible difference caused by variations of the chemical composition in the envelope.
Key words: stars: neutron / stars: magnetic fields / dense matter / conduction / pulsars: general
© ESO, 2005
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