The effect of rotational gravity darkening on magnetically torqued Be star discs

Monthly Notices of the Royal Astronomical Society

Volumn 352, Issue 3, 2004, Pages 1061-1072

  Brown, J C ^a   Telfer, D ^a   Li, Q ^a,b   Hanuschik, R ^c   Cassinelli, J P ^d   Kholtygin, A ^e,f  

^a UNIVERSITY OF GLASGOW   (United Kingdom)

^b BEIJING NORMAL UNIVERSITY   (China)

^c EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^d UNIVERSITY OF WISCONSIN MADISON   (United States)

^e ST PETERSBURG STATE UNIVERSITY   (Russian Federation)

^f Branch in St Petersburg   (Russian Federation)

Author keywords

Polarization; Stars: emission line, Be; Stars: magnetic fields; Stars: mass loss stars: rotation; Stars: winds, outflows

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; GRAVITATION; STARS; WIND;

BE STARS; DISK MODEL; MASS-LOSS - STARS; STAR: MASS-LOSS-STAR: ROTATION; STARS: EMISSION-LINE BE; STARS: MAGNETIC FIELD; STARS: MASS-LOSS; STARS: ROTATION; STARS: WINDS OUTFLOWS; STELLARS;

POLARIZATION;

EID: 4043058026     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07997.x     Document Type: Article

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