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2016ApJ...824..143L - Astrophys. J., 824, 143-143 (2016/June-3)
Can the subsonic accretion model explain the spin period distribution of wind-fed X-ray pulsars?
LI T., SHAO Y. and LI X.-D.
Abstract (from CDS):
Abstract Copyright: © 2016. The American Astronomical Society. All rights reserved.
Journal keyword(s): stars: early-type - stars: evolution - stars: neutron - X-rays: binaries
Simbad objects: 13
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