Be-star rotation: How close to critical?

Monthly Notices of the Royal Astronomical Society

Volumn 350, Issue 1, 2004, Pages 189-195

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

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b UNIVERSITY OF DELAWARE   (United States)

Author keywords

Line: profiles; Stars: emission line, Be; Stars: fundamental parameters; Stars: rotation; Techniques: spectroscopic

Indexed keywords

STARS;

BE STARS; GRAVITY DARKENING; LINE-WIDTH; LINE: PROFILES; OBSERVATIONAL STUDY; PROFILE CALCULATION; STARS: EMISSION-LINE BE; STARS: ROTATION; STARS:FUNDAMENTAL PARAMETERS; TECHNIQUES: SPECTROSCOPIC;

ROTATION;

EID: 2442488746     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07627.x     Document Type: Article

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