Orbital parameters of binary radio pulsars in globular clusters and stellar interactions

Details Orbital parameters of binary radio pulsars in globular clusters and stellar interactions Orbital parameters of binary radio pulsars in globular clusters and stellar interactions

2009-09-16

arxiv.org/abs/0909.3062v1

ASPC 407 (2009) 353

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Published in the Low-Frequency Radio Universe ASP Conference Series, Vol. 407, proceedings of the conference held 8-12 Decembe

Scientific paper

The observed distribution of globular cluster binary radio pulsars in the eccentricity versus orbital period plane can be explained as a result of binary-single star interactions. Our numerical and analytical study hints that the highest eccentricity binaries in clusters are likely to be from exchange and/or merger of a single star with a binary component, while the intermediate eccentricity systems are probably results of fly-by interactions.

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