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The death line of millisecond pulsars

Published online by Cambridge University Press:  12 April 2016

Claes-Ingvar Björnsson
Claes-Ingvar Björnsson*
Affiliation:
Stockholm, Observatory, S-133 36 Saltsjöbaden, Sweden

Abstract

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The distribution of millisecond pulsars, just as normal pulsars, is affected by a death line. Since a large fraction of millisecond pulsars lie close to the derived death line, a significant number of neutron stars may exist which are not observed as millisecond pulsars. This makes the birth rate discrepancy between millisecond pulsars and their assumed low mass x-ray binary progenitors more acute.

Type
Part 3 Radio Emission Processes
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 189 - 190
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

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