On the existence of low-luminosity cataclysmic variables beyond the orbital period minimum

Monthly Notices of the Royal Astronomical Society

Volumn 287, Issue 4, 1997, Pages 929-936

  Howell, Steve B ^a   Rappaport, Saul ^b   Politano, Michael ^c  

^a UNIVERSITY OF WYOMING   (United States)

^b MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^c ARIZONA STATE UNIVERSITY   (United States)

Author keywords

Binaries: close; Galaxy: evolution; Novae, cataclysmic variables; Stars: low mass, brown dwarfs

Indexed keywords

LUMINANCE; MASS TRANSFER; STARS;

BINARIES: CLOSE; BROWN DWARFS; CATACLYSMIC VARIABLES; DWARF NOVAE; GALAXY EVOLUTION; LOW-MASS; MASS TRANSFER RATE; NOVAE CATACLYSMIC VARIABLES; ORBITAL PERIODS; STARS: LOW-MASS BROWN DWARFS;

GALAXIES;

EID: 0001246176     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/287.4.929     Document Type: Article

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