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Neutron Star Cooling and the Vela Pulsar

Published online by Cambridge University Press:  04 August 2017

Ken'ichi Nomoto  and
Sachiko Tsuruta
Ken'ichi Nomoto
Affiliation:
1Physics Department, Brookhaven National Laboratory; on leave from the Department of Earth Science and Astronomy, University of Tokyo
Sachiko Tsuruta
Affiliation:
2Department of Physics, Montana State University

Extract

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We have calculated cooling models of young neutron stars.3 The theoretical cooling curves for several models are compared with the Einstein X-ray observations of young supernova remnants (Figure 1).

Type
V. Neutron Star Physics
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 456
Copyright
Copyright © Reidel 1987