Constraining the Neutron Star Mass-Radius Relation and Dense Matter Equation of State with NICER. II. Emission from Hot Spots on a Rapidly Rotating Neutron Star
We describe the model of surface emission from a rapidly rotating neutron star that is applied to Neutron Star Interior Composition Explorer X-ray data of millisecond pulsars in order to statistically constrain the neutron star mass-radius relation and dense matter equation of state. To ensure that...
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Other Authors: | , |
Format: | Article |
Language: | English |
Published: |
American Astronomical Society,
2020-06-08T20:07:02Z.
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Subjects: | |
Online Access: | Get fulltext |