The distributions of neutron star and black-hole masses are analyzed to provide constraints on models of the neutron star equation of state. Inclinations obtained from ellipsoidal analysis and the excess noise seen in SXT light curves, are discussed.
| Identifer | oai:union.ndltd.org:bl.uk/oai:ethos.bl.uk:360365 |
| Date | January 1995 |
| Creators | Martin, Andrew Charles |
| Publisher | University of Oxford |
| Source Sets | Ethos UK |
| Detected Language | English |
| Type | Electronic Thesis or Dissertation |
| Source | http://ora.ox.ac.uk/objects/uuid:6c442538-1820-4a4b-b002-923799340481 |
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