Abstract
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.
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Funding
The work of A.V. Yudin and S.I. Blinnikov was supported by the Russian Foundation for Basic Research (project no. 18-29-021019 mk).
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Russian Text © The Author(s), 2019, published in Pis’ma v Astronomicheskii Zhurnal, 2019, Vol. 45, No. 12, pp. 893–901.
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Yudin, A.V., Razinkova, T.L. & Blinnikov, S.I. Low-Mass Neutron Stars with Rotation. Astron. Lett. 45, 847–854 (2019). https://doi.org/10.1134/S1063773719120077
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DOI: https://doi.org/10.1134/S1063773719120077