Measuring the stellar wind parameters in IGR J17544-2619 and Vela X-1 constrains the accretion physics in supergiant fast X-ray transient and classical supergiant X-ray binaries-Reference-Cited by-同舟云学术

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Measuring the stellar wind parameters in IGR J17544-2619 and Vela X-1 constrains the accretion physics in supergiant fast X-ray transient and classical supergiant X-ray binaries

Published:2016-06-06 Issue: Volume:591 Page:A26
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Giménez-García A.,Shenar T.,Torrejón J. M.,Oskinova L.,Martínez-Núñez S.,Hamann W.-R.,Rodes-Roca J. J.,González-Galán A.,Alonso-Santiago J.,González-Fernández C.,Bernabeu G.,Sander A.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201527551/pdf

Reference106 articles.

1. The Chemical Composition of the Sun

2. INTEGRAL observations of the variability of OAO 1657-415

3. The mass of the neutron star in Vela X-1

4. NuSTAR detection of a cyclotron line in the supergiant fast X-ray transient IGR J17544−2619

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