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Paper: Orbital Parameters of Binary Radio Pulsars in Globular Clusters and Stellar Interactions
Volume: 407, The Low-Frequency Radio Universe
Page: 353
Authors: Bagchi,M.; Ray, A.
Abstract: 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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