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Recovery of the X‐Ray Transient QX Normae (=X1608−52) in Outburst and Quiescence
Author(s) -
Stefanie Wachter
Publication year - 1997
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/304463
Subject(s) - astrophysics , physics , transient (computer programming) , magnitude (astronomy) , binary number , astronomy , arithmetic , mathematics , computer science , operating system
We present optical and near-IR observations of QX Nor, the counterpart to therecurrent soft X-ray transient X1608-52, after its reappearance following theX-ray outburst in February 1996. The object has been seen only once before,during an X-ray outburst in 1977. Data from 3-5 months after the outburst showthe counterpart at a mean magnitude of R=20.2 and variable on timescales ofdays. A comparison with identical observations in 1995 implies that the objecthas brightened by at least 1.8 mag in R following the X-ray outburst. We alsodetected QX Nor in the IR in both quiescence and outburst. A faint source isvisible in the J but not the R band in May 1995. These first observations inthe quiescent state yield magnitudes and colors consistent with opticalemission from a low mass companion in the binary system, as is true in othersoft X-ray transients.Comment: 10 pages including 4 figures and 2 tables; Uses AASTeX 4.0; Accepted for publication in The Astrophysical Journal, Volume 485, August 20, 199

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