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Pulse Asymmetry of Millisecond Pulsars

Published online by Cambridge University Press:  04 August 2017

Kai You Chen  and
Jacob Shaham
Kai You Chen
Affiliation:
Columbia Astrophysics Laboratory and Department of Physics, Columbia University New York, New York 10027
Jacob Shaham
Affiliation:
Columbia Astrophysics Laboratory and Department of Physics, Columbia University New York, New York 10027

Abstract

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By considering a simple model of slowly rotating neutron stars (for which the Schwartzschild metric could be used properly) whose emission is confined to circular antipolar caps, Pechenick, Ftaclas and Cohen (1983) studied the gravitational effects on the light curves. They found that for typical neutron star parameters, the light curves flattened out due to the bending of light in the neutron stellar gravity.

Type
I. Rotation-Powered Pulsars
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 55
Copyright
Copyright © Reidel 1987