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SW Sextantis stars: the dominant population of cataclysmic variables with orbital periods between 3 and 4 h
2007
86 citations
Journal Article
bronze Open Access
Field-Weighted Citation Impact:
3.62
SW Sextantis stars: the dominant population of cataclysmic variables with orbital periods between 3 and 4 h | Researchclopedia
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British Astronomical Association
J. Casares
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Instituto de Astrofísica de Canarias
D. Engels
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Universität Hamburg
Omiros Giannakis
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National Observatory of Athens
E. T. Harlaftis
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National Observatory of Athens
J. Kube
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Alfred-Wegener-Institut Helmholtz-Zentrum für Polar- und Meeresforschung
H. J. Lehto
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University of Turku
I. G. Martínez-Pais
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Universidad de La Laguna
R. Schwarz
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Leibniz Institute for Astrophysics Potsdam
Warren Skidmore
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California Institute of Technology
A. Staude
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Leibniz Institute for Astrophysics Potsdam
M. A. P. Torres
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Center for Astrophysics Harvard & Smithsonian