Cataclysmic Variables from SDSS II. The Second Year

• Published in: arXiv.org
• Main Authors: Szkody, Paula, Fraser, Oliver, Silvestri, Nicole, Henden, Arne, Anderson, Scott F, Frith, James, Lawton, Brandon, Owens, Ethan, Raymond, Sean, Schmidt, Gary, Wolfe, Michael, Bochanski, John, Covey, Kevin, Harris, Hugh, Hawley, Suzanne, Knapp, Gillian R, Margon, Bruce, Voges, Wolfgang, Walkowicz, Lucianne, Brinkmann, J, Lamb, D Q
• Format: Paper
• Language: English
• Published: Ithaca Cornell University Library, arXiv.org 16.08.2003
• Subjects: Cataclysmic variables; Curves; Deposition; Dwarf novae; Mass transfer; Orbits; Quasars; Sky surveys (astronomy); Spectra
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.0306269

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.