MODELING THE X-RAYS FROM THE CENTRAL COMPACT OBJECT PSR J1852+0040 IN KESTEVEN 79: EVIDENCE FOR A STRONGLY MAGNETIZED NEUTRON STAR-Reference-Cited by-同舟云学术

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MODELING THE X-RAYS FROM THE CENTRAL COMPACT OBJECT PSR J1852+0040 IN KESTEVEN 79: EVIDENCE FOR A STRONGLY MAGNETIZED NEUTRON STAR

Published:2014-07-09 Issue:2 Volume:790 Page:94
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Bogdanov Slavko^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/790/i=2/a=94/pdf

Reference70 articles.

1. Gravitational Bending of Light Near Compact Objects

2. HYPERCRITICAL ACCRETION ONTO A NEWBORN NEUTRON STAR AND MAGNETIC FIELD SUBMERGENCE

3. The magnetic field of an isolated neutron star from X-ray cyclotron absorption lines

4. Hypercritical spherical accretion onto compact objects

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