REFINED ORBITAL SOLUTION AND QUIESCENT VARIABILITY IN THE BLACK HOLE TRANSIENT GS 1354-64 (= BW Cir)

REFINED ORBITAL SOLUTION AND QUIESCENT VARIABILITY IN THE BLACK HOLE TRANSIENT GS 1354-64 (= BW Cir)

In Casares et al. we presented the first radial velocity curve of the companion star to BW Cir which demonstrates the presence of a black hole in this historical X-ray transient. But these data were affected by aliasing and two possible periods at 2.5445 days and 2.5635 days were equally possible. H...

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Main Authors: Casares, J. (Author), Orosz, Jerome A. (Author), Zurita, C. (Author), Shahbaz, T. (Author), Corral-Santana, J. M. (Author), McClintock, Jeffrey E. (Author), Garcia, M. R. (Author), Martínez-Pais, I. G. (Author), Charles, P. A. (Author), Fender, R. P. (Author), Remillard, Ronald A (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor), Remillard, Ronald Alan (Contributor)
Format: Article
Language:English
Published: Institute of Physics/American Astronomical Society, 2015-03-05T21:05:55Z.
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