SW Sextantis stars: the dominant population of cataclysmic variables with orbital periods between 3 and 4 h |
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Authors: | P. Rodrí guez-Gil,B. T. Gä nsicke,H.-J. Hagen,S. Araujo-Betancor,A. Aungwerojwit,C. Allende Prieto,D. Boyd,J. Casares,D. Engels,O. Giannakis,E. T. Harlaftis,J. Kube,H. Lehto,I. G. Martí nez-Pais,R. Schwarz,W. Skidmore,A. Staude, M. A. P. Torres |
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Affiliation: | Instituto de Astrofísica de Canarias, Vía Láctea s/n, La Laguna, E-38205 Santa Cruz de Tenerife, Spain;Department of Physics, University of Warwick, Coventry CV4 7AL;Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany;Department of Physics, Faculty of Science, Naresuan University, Phitsanulok 65000, Thailand;McDonald Observatory and Department of Astronomy, University of Texas, Austin, TX 78712, USA;British Astronomical Association, Variable Star Section, West Challow OX12 9TX;Institute of Astronomy and Astrophysics, National Observatory of Athens, PO Box 20048, Athens 11810, Greece;Institute of Space Applications and Remote Sensing, National Observatory of Athens, PO Box 20048, Athens 11810, Greece;Alfred-Wegener-Institut für Polar- und Meeresforschung, Bürgermeister-Smidt-Straße 20, 27568 Bremerhaven, Germany;Tuorla Observatory, University of Turku, FIN-21500 Piikkiö, Finland;Department of Physics, FIN-20014 University of Turku, Finland;Departamento de Astrofísica, Universidad de La Laguna, Tenerife, Spain;Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany;California Institute of Technology, Mail Code 105-24, Pasadena, CA 91125-24, USA;Harvard–Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA |
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Abstract: | |
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Keywords: | accretion, accretion discs binaries: close novae, cataclysmic variables |
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