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