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SW Sextantis stars: the dominant population of cataclysmic variables with orbital periods between 3 and 4 h

SW Sextantis stars: the dominant population of cataclysmic variables with orbital periods between 3 and 4 h

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
  • 作者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
  • 卷第377卷
  • 期第4期
  • 印刷ISSN0035-8711
  • 电子ISSN1365-2966
  • 文件大小1485.89KB
  • 发表时间2007
  • DOI10.1111/j.1365-2966.2007.11743.x
  • 页码1747-1762
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