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The quasi-persistent neutron star soft X-ray transient 1M 1716−315 in quiescence
Authors:P. G. Jonker  C. G. Bassa   S. Wachter
Affiliation:SRON, Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA, Utrecht, the Netherlands;Harvard-Smithsonian Centre for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA;Astronomical Institute, Utrecht University, PO Box 80000, 3508 TA, Utrecht, the Netherlands;Spitzer Science Center, California Institute of Technology, 1200 E. California Blvd., Pasadena CA 91125, USA
Abstract:
Keywords:accretion: accretion discs    stars: individual: 1M 1716−315 - binaries: general    stars: neutron    X-rays: binaries
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