FURTHER EVIDENCE FOR THE BIMODAL DISTRIBUTION OF NEUTRON-STAR MASSES
We use a collection of 14 well-measured neutron-star masses to strengthen the case that a substantial fraction of these neutron stars were formed via electron-capture (e-capture) supernovae (SNe) as opposed to Fe core-collapse SNe. The e-capture SNe are characterized by lower resultant gravitational...
Main Authors: | , , |
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Other Authors: | , , |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2015-02-26T20:18:13Z.
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Subjects: | |
Online Access: | Get fulltext |