Low-Mass Neutron Stars with Rotation

The properties of low-mass neutron stars with rigid rotation are considered. The possible evolution paths of such stars in a close binary system with mass transfer are calculated. The properties of the gamma-ray burst GRB 170817A interpreted in terms of the stripping model, a natural ingredient of w...

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Bibliographic Details
Published in:Astronomy letters 2019-12, Vol.45 (12), p.847-854
Main Authors: Yudin, A. V., Razinkova, T. L., Blinnikov, S. I.
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics and Astroparticles
Binary stars
Gamma ray bursts
Gamma rays
Mass transfer
Neutron stars
Neutrons
Observations and Techniques
Physics
Physics and Astronomy
Stellar evolution
Stellar rotation
Stellar system evolution
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Summary:The properties of low-mass neutron stars with rigid rotation are considered. The possible evolution paths of such stars in a close binary system with mass transfer are calculated. The properties of the gamma-ray burst GRB 170817A interpreted in terms of the stripping model, a natural ingredient of which is the explosion of a low-mass neutron star—a binary component, are briefly discussed.
ISSN:1063-7737
1562-6873
DOI:10.1134/S1063773719120077