Cataclysmic Variables from Sloan Digital Sky Survey. V. The Fifth Year (2004)
The Astronomical Journal2006Vol. 131(2), pp. 973–983
Citations Over TimeTop 10% of 2006 papers
Paula Szkody, A. A. Henden, Marcel A. Agüeros, Scott F. Anderson, John J. Bochanski, G. R. Knapp, Lee Mannikko, Anjum S. Mukadam, Nicole M. Silvestri, Gary D. Schmidt, Brian Stephanik, T. K. Watson, Andrew A. West, D. E. Winget, M. A. Wolfe, John C. Barentine, J. Brinkmann, H. Brewington, R. A. Downes, Michael Harvanek, S. J. Kleinman, J. Krzesiński, Dan Long, Eric H. Neilsen, A. Nitta, Donald P. Schneider, Stephanie A. Snedden, W. Voges
Abstract
This paper identifies the cataclysmic variables that appear in spectra obtained in 2004 as part of the Sloan Digital Sky Survey. Spectra of 41 objects, including seven systems that were previously known (CC Cnc, DW Cnc, PQ Gem, AR UMa, AN UMa, RX J1131.3+4322, and UMa 6) and 34 new cataclysmic variables are presented. The positions and ugriz photometry of all 41 systems are given, as well as additional follow-up spectroscopic, photometric, and/or polarimetric observations of eight of the new systems. The new objects include three eclipsing systems, six with prominent He II emission, and six systems that show the underlying white dwarf.
Related Papers
- → Evidence for pole switching in the magnetic cataclysmic variable BY Camelopardalis(1998)38 cited
- → White Dwarfs in Cataclysmic Variables: An Update(2015)1 cited
- → The Effect of the Nova Explosion on the Evolution of Cataclysmic Variables(1997)
- → Gaia, an all sky astrometric and photometric survey(2017)
- → The Effective Temperature Distribution Function of Cataclysmic Variable White Dwarfs(1987)