Cataclysmic variables with evolved secondaries and the progenitors of AM CVn stars

Monthly Notices of the Royal Astronomical Society

Volumn 340, Issue 4, 2003, Pages 1214-1228

  Podsiadlowski, Ph ^a   Han, Z ^b   Rappaport, S ^c  

^a UNIVERSITY OF OXFORD   (United Kingdom)

^b Chinese Academy of Sciences   (China)

^c MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Binaries: close; Gravitation; Novae, cataclysmic variables; White dwarfs

Indexed keywords

EFFICIENCY; MASS TRANSFER;

BINARIES: CLOSE; CATACLYSMIC VARIABLES; NOVAE CATACLYSMIC VARIABLES; ORBITAL PERIODS; POPULATION SYNTHESIS; RELATED SYSTEMS; STELLAR EVOLUTIONS; SYNTHESIS MODELS; SYSTEMATIC STUDY; VARIABLE SYSTEMS;

WHITE DWARFS;

EID: 0141429831     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06380.x     Document Type: Article

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