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24 April 2024
 
  » arxiv » 1101.1513

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The New Eclipsing Cataclysmic Variable SDSS 154453+2553
Julie N. Skinner ; John R. Thorstensen ; Eve Armstrong ; Steve Brady ;
Date 7 Jan 2011
AbstractThe 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 H{alpha} 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.
Source arXiv, 1101.1513
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