Formation and Evolution of Neutron Star Binaries: Masses of Neutron Stars

Neutron star (NS) is one of the most interesting astrophysical compact objects for hardronic physics. It is believed that the central density of NS can reach several times the normal nuclear matter density (ρ0). Hence, the inner part of NS is the ultimate testing place for the physics of dense matte...

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Bibliographic Details
Main Author: Lee Chang-Hwan
Format: Article
Language:English
Published: EDP Sciences 2012-02-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20122004002

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