Swift J1753.5−0127: The Black Hole Candidate with the Shortest Orbital Period-Reference-Cited by-同舟云学术

Swift J1753.5−0127: The Black Hole Candidate with the Shortest Orbital Period

Published:2008-07-10 Issue:2 Volume:681 Page:1458-1463
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Zurita C.,Durant M.,Torres M. A. P.,Shahbaz T.,Casares J.,Steeghs D.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference45 articles.

1. Periodic variability in the optical counterpart of X-ray Nova MUSCAE 1991

2. “Soft X-ray transient” outbursts which are not soft

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

4. Cadolle Bel, M., Ribo, M., Rodriguez, J., Chaty, S., Corbel, S., Goldwurm, A. & Malzac, J. 2006, in Microquasars and Beyond, ed. T. Belloni (Trieste: SISSA), 3

5. Simultaneous Multiwavelength Observations of the Low/Hard State of the X‐Ray Transient Source SWIFT J1753.5−0127

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