Low-Mass Neutron Stars with Rotation
High Energy Astrophysical Phenomena
2020-05-12 v1 Solar and Stellar Astrophysics
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.
Cite
@article{arxiv.2005.04428,
title = {Low-Mass Neutron Stars with Rotation},
author = {A. V. Yudin and T. L. Razinkova and S. I. Blinnikov},
journal= {arXiv preprint arXiv:2005.04428},
year = {2020}
}
Comments
16 pages, 3 figs, 1 table