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arXiv · 1101.1513

The New Eclipsing Cataclysmic Variable SDSS 154453+2553

Julie N. Skinner·John R. Thorstensen·Eve Armstrong·Steve Brady
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Abstract

The cataclysmic variable SDSS154453+2553 was recently identified in the Sloan Digital Sky Survey. We obtained spectra and photometry at the MDM Observatory, which revealed an eclipse with a 6.03 hour period. The Hα emission line exhibits a strong rotational disturbance during eclipse, indicating that it arises in an accretion disk. A contribution from an M-type companion is also observed. Time-series photometry during eclipse gives an ephemeris of 2454878.0062(15) + 0.251282(2)E. We present spectroscopy through the orbit and eclipse photometry. Our analysis of the secondary star indicates a distance of 800 {\pm} 180 pc.

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Julie N. Skinner, John R. Thorstensen, Eve Armstrong, Steve Brady. 2011-01-07. The New Eclipsing Cataclysmic Variable SDSS 154453+2553. https://doi.org/10.1086/658878

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