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SW Sextantis stars: the dominant population of cataclysmic variables with orbital periods between 3 and 4 h
Authors:P Rodríguez-Gil  B T Gänsicke  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 Martínez-Pais  R Schwarz  W Skidmore  A Staude  M A P Torres
Institution: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
Abstract:
Keywords:accretion  accretion discs  binaries: close  novae  cataclysmic variables
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