X-ray Nova XTE J1550-564: Optical Observations
arXiv:astro-ph/9903398 · doi:10.1086/312041
Abstract
We report the identification of the optical counterpart of the X-ray transient XTE J1550-564 described in two companion papers by Sobczak et al (1999) and Remillard et al (1999). We find that the optical source brightened by approximately 4 magnitudes over the quiescent counterpart seen at B~22 on a SERC survey plate, and then decayed by approximately 1.5 magnitudes over the 7 week long observation period. There was an optical response to the large X-ray flare described by Sobczak et al (1999), but it was much smaller and delayed by roughly 1 day.
9 pages, 2 figures. Accepted for publication in ApJ Letters
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Cited by in corpus (24)
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- Coronal X-Ray Emission from the Stellar Companions to Transiently Accreting Black Holes
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- NIR and optical observations of the failed outbursts of black hole binary XTE J1550-564
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