Optical Time-Series Photometry of the Peculiar Nova CSS081007:030559+054715

Details Optical Time-Series Photometry of the Peculiar Nova CSS081007:030559+054715 Optical Time-Series Photometry of the Peculiar Nova CSS081007:030559+054715

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010javso..38..147t&link_type=abstract

The Journal of the American Association of Variable Star Observers, vol. 38, nr. 2, p. 147

Physics

Scientific paper

We present an analysis of optical photometry of the transient optical and X-ray source CSS081007:030559+054715. Unfiltered CCD observations were made between 2008 December 17 and December 30 (JD 2454817.5 to 2454830.5), showing variability at the level of 0.5 magnitude. Time-series analyses of these data confirm the existence of the 1.77-day period detected in X-ray, UV, and optical wavelengths by te Swift satellite. The maxima of the optical and X-ray emission appear to be out of phase.

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