arXiv · astro-ph/0306269
Cataclysmic Variables from SDSS II. The Second Year
Abstract
The first full year of operation following the commissioning year of the Sloan Digital Sky Survey has revealed a wide variety of newly discovered cataclysmic variables. We show the SDSS spectra of forty-two cataclysmic variables observed in 2002, of which thirty-five are new classifications, four are known dwarf novae (CT Hya, RZ Leo, T Leo and BZ UMa), one is a known CV identified from a previous quasar survey (Aqr1) and two are known ROSAT or FIRST discovered CVs (RX J09445+0357, FIRST J102347.6+003841). The SDSS positions, colors and spectra of all forty-two systems are presented. In addition, the results of follow-up studies of several of these objects identify the orbital periods, velocity curves and polarization that provide the system geometry and accretion properties. While most of the SDSS discovered systems are faint (>18th mag) with low accretion rates (as implied from their spectral characteristics), there are also a few bright objects which may have escaped previous surveys due to changes in the mass transfer rate.
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Paula Szkody, Oliver Fraser, Nicole Silvestri, Arne Henden, Scott F. Anderson, James Frith, Brandon Lawton, Ethan Owens, Sean Raymond, Gary Schmidt, Michael Wolfe, John Bochanski, Kevin Covey, Hugh Harris, Suzanne Hawley, Gillian R. Knapp, Bruce Margon, Wolfgang Voges, Lucianne Walkowicz, J. Brinkmann, D. Q. Lamb. 2003-08-16. Cataclysmic Variables from SDSS II. The Second Year. https://doi.org/10.1086/377346
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