A rigidly rotating magnetosphere model for circumstellar emission from magnetic OB stars

Monthly Notices of the Royal Astronomical Society

Volumn 357, Issue 1, 2005, Pages 251-264

  Townsend, R H D ^a,b   Owocki, S P ^a  

^a UNIVERSITY OF DELAWARE   (United States)

^b UNIVERSITY COLLEGE LONDON   (United Kingdom)

Author keywords

Stars: chemically peculiar; Stars: early type; Stars: emission line, Be; Stars: magnetic fields; Stars: mass loss; Stars: rotation

Indexed keywords

BLACK HOLES; GRAVITATION; MAGNETIC FIELDS; MAGNETOSPHERE; RIGIDITY;

CIRCUMSTELLAR; FIELD LINES; MAGNETOSPHERE MODEL; ROTATION AXES; STARS: CHEMICALLY PECULIAR; STARS: EMISSION-LINE BE; STARS: MAGNETIC FIELD; STARS: MASS-LOSS; STARS: ROTATION; STARS:EARLY TYPE;

STARS;

EID: 13744259338     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.08642.x     Document Type: Article

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