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CAN THE SUBSONIC ACCRETION MODEL EXPLAIN THE SPIN PERIOD DISTRIBUTION OF WIND-FED X-RAY PULSARS?

By Tao Li, Yong Shao and Xiang-Dong Li
Publisher: American Astronomical Society
Year: 2016
DOI identifier: 10.3847/0004-637x/824/2/143
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Provided by: MUCC (Crossref)
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