Evidence of a Black Hole in the X-Ray Transient GS 1354-64 (=BW Circini)-Reference-Cited by-同舟云学术

Evidence of a Black Hole in the X-Ray Transient GS 1354-64 (=BW Circini)

Published:2004-08-23 Issue:2 Volume:613 Page:L133-L136
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Casares J.,Zurita C.,Shahbaz T.,Charles P. A.,Fender R. P.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference25 articles.

1. Linearized limb-darkening coefficients for use in analysis of eclipsing binary light curves

2. The 1997 hard-state outburst of the X-ray transient GS 1354-64/BW Cir

3. A 6.5-day periodicity in the recurrent nova V404 Cygni implying the presence of a black hole

4. Charles, P. A. & Coe, M. J. 2004, in Compact Stellar X-Ray Sources, ed. W. H. G. Lewin & M. van der Klis (Cambridge: Cambridge Univ. Press), in press (astro-ph/0308020)

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