Pulsar Population Synthesis

Details Pulsar Population Synthesis Pulsar Population Synthesis

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...189.7409w&link_type=abstract

American Astronomical Society, 189th AAS Meeting, #74.09; Bulletin of the American Astronomical Society, Vol. 28, p.1369

Astronomy and Astrophysics

Astronomy

Scientific paper

We present results of the kinematics of the pulsar population using Monte Carlo simulations and a revised (and corrected) form of the Lyne and Lorimer birth velocity distribution. We discuss how the initial birth properties are constrained by observations. As a corollary we explore the hypothesis that the isolated millisecond pulsar population is a subset of the "regular" population whose members lie on the low end tail of the magnetic field distribution.

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