The orbital period of the dwarf nova HS Virginis, the revised Po - Ps relation and the "superhump" mass ratio distribution of SU UMa stars

Astronomy and Astrophysics

Volumn 348, Issue 2, 1999, Pages 466-474

  Mennickent, R E ^a,d   Matsumoto, K ^b   Arenas, J ^c  

^a UNIVERSITY OF CONCEPCIÓN   (Chile)

^b KYOTO UNIVERSITY   (Japan)

^c KEELE UNIVERSITY   (United Kingdom)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Stars: evolution stars: binaries: general; Stars: Fundamental parameters; Stars: Individual: HS Vir; Stars: novae, cataclysmic variables

Indexed keywords

EID: 0000137772     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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