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On the spin evolution of neutron stars in pre-low-mass X-ray binaries

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 09 Apr 2004Embargo end date: 01 Jan 2003Publisher:EDP SciencesJournal:Astronomy & Astrophysics, volume 418, pages 699-702 (issn: 0004-6361, eissn: 1432-0746,

Authors: Sergei Popov; Sergei Popov;

doi: 10.1051/0004-6361:20035695 , 10.48550/arxiv.astro-ph/0311521

arXiv: http://arxiv.org/abs/astro-ph/0311521

On the spin evolution of neutron stars in pre-low-mass X-ray binaries

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Abstract

We present a simple model for the evolutionary states of neutron stars in pre-low-mass X-ray binaries during the main sequence stage of donor stars. It is shown that for typical parameters some of the neutron stars in these systems can not accrete matter from winds of their companions in a stable way. Accretors are found if neutron stars have magnetic fields about $10^{13}$ G and higher and/or in close systems with orbital periods about a few days and shorter.

4 pages, 2 figures; revised version

Related Organizations

University of Padua
Italy
Sternberg Astronomical Institute
Russian Federation
University of Management TISBI
Russian Federation

Keywords

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

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NEANIAS Space Research Community