Ryan S. Lynch, Jason R. Boyles, Duncan R. Lorimer, Robert Mnatsakanov, Philip J. Turk, Scott M. Ransom
Published 2011-01-04Version 1
We place limits on the population of non-recycled pulsars originating in globular clusters through Monte Carlo simulations and frequentist statistical techniques. We set upper limits on the birth rates of non-recycled cluster pulsars and predict how many may remain in the clusters, and how many may escape the cluster potentials and enter the field of the Galaxy.
Comments: 3 pages, to appear in proceedings of "Radio Pulsars: An astrophysical key to unlock the secrets of the Universe"
Inverting the dynamical evolution of globular clusters: clues to their origin
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The Galactic evolution of sulphur as traced by globular clusters
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