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          Institute: MPI für extraterrestrische Physik     Collection: High Energy Astrophysics at MPE     Display Documents



ID: 5955.0, MPI für extraterrestrische Physik / High Energy Astrophysics at MPE
Cataclysmic variables from the Sloan Digital Sky Survey. I. The first results
Authors:Szkody, Paula; Anderson, Scott F.; Agüeros, Marcel; Covarrubias, Ricardo; Bentz, Misty; Hawley, Suzanne; Margon, Bruce; Voges, Wolfgang; Henden, Arne; Knapp, Gillian R.; Vanden Berk, Daniel E.; Rest, Armin; Miknaitis, Gajus; Magnier, Eugene; Brinkmann, J.; Csabai, I.; Harvanek, M.; Hindsley, R.; Hennessy, G.; Ivezic, Z.; Kleinman, S. J.; Lamb, D. Q.; Long, D.; Newman, P. R.; Neilsen, E. H.; Nichol, R. C.; Nitta, A.; Schneider, D. P.; Snedden, S. A.; York, D. G.
Language:English
Date of Publication (YYYY-MM-DD):2002-01
Title of Journal:The Astronomical Journal
Journal Abbrev.:Astron. J.
Volume:123
Issue / Number:1
Start Page:430
End Page:442
Review Status:Peer-review
Audience:Experts Only
Abstract / Description:The commissioning year of the Sloan Digital Sky Survey (SDSS) has demonstrated that many cataclysmic variables (CVs) have been missed in previous surveys with brighter limits. We report the identification of 22 CVs, of which 19 are new discoveries and three are known systems ( SW UMa, BH Lyn, and OU Vir). A compendium of positions, colors, and characteristics of these systems obtained from the SDSS photometry and spectroscopy is presented, along with data obtained during follow-up studies with the Apache Point Observatory and Manastash Ridge Observatory telescopes. We have determined orbital periods for three of the new systems, two show dwarf nova outbursts, and the third is a likely magnetic system with eclipses of its region of line emission. Based on these results, we expect the completed survey to locate at least 400 new CVs. Most of these will be faint systems with low accretion rates that will provide new constraints on binary evolution models.
Free Keywords:novae; cataclysmic variables; techniques : photometric; techniques : spectroscopic
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für extraterrestrische Physik
External Affiliations:Univ Washington, Dept Astron, Box 351580, Seattle, WA 98195 USA; Univ Washington, Dept Astron, Seattle, WA 98195 USA; Space Telescope Sci Inst, Baltimore, MD 21218 USA; Max Planck Inst Extraterr Phys, D-85741 Garching, Germany; USN Observ, Univ Space Res Assoc, Flagstaff Stn, Flagstaff, AZ 86002 USA; Princeton Univ Observ, Princeton, NJ 08544 USA; Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA; Apache Point Observ, Sunspot, NM 88349 USA; Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA; USN Observ, Washington, DC 20392 USA; Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA; Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA; Carnegie Mellon Univ, Dept Phys, Pittsburgh, PA 15232 USA; Penn State Univ, Dept Astron & Astrophys, Davey Lab 525, University Pk, PA 16802 USA
Identifiers:ISI:000173767400033
ISSN:0004-6256
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