SIMBAD references

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):

Neutron stars in high-mass X-ray binaries (HMXBs) generally accrete from the wind matter of their massive companion stars. Recently, Shakura et al. suggested a subsonic accretion model for low-luminosity (

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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