The origin of subdwarf B stars - II

Monthly Notices of the Royal Astronomical Society

Volumn 341, Issue 2, 2003, Pages 669-691

  Han, Z ^a   Podsiadlowski, Ph ^b   Maxted, P F L ^c   Marsh, T R ^d  

^a CHINESE ACADEMY OF SCIENCES   (China)

^b UNIVERSITY OF OXFORD   (United Kingdom)

^c KEELE UNIVERSITY   (United Kingdom)

^d UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

Author keywords

Binaries: Close; Subdwarfs; White dwarfs

Indexed keywords

GALAXIES; GRAVITATION; HELIUM; MASS TRANSFER; MERGING; POPULATION STATISTICS; TEMPERATURE;

BEST ESTIMATES; BINARIES: CLOSE; BINARY FRACTION; ORBITAL PERIODS; POPULATION SYNTHESIS; SUBDWARFS; SYNTHESIS CODE; SYNTHESIS MODELS; TWO PHASE; WORKERS';

WHITE DWARFS;

EID: 0141946170     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06451.x     Document Type: Article

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