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Astronomy and Astrophysics

Volumn 383, Issue 1, 2002, Pages 218-226

Spin-up of Be stars in the pre-main sequence phase

(1) Stepien, K a,b

a UNIVERSITY OF WESTERN ONTARIO (Canada)

b UNIVERSITY OF WARSAW (Poland)

Author keywords

Stars: emission line, Be; Stars: magnetic fields; Stars: pre main sequence; Stars: rotation

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; MAGNETIC FIELD EFFECTS; MAGNETIC FLUX; MATHEMATICAL MODELS; WIND EFFECTS;

STARS;

ASTROPHYSICS;

EID: 0036472611 PISSN: 00046361 EISSN: None Source Type: Journal
DOI: 10.1051/0004-6361:20011695 Document Type: Article

Times cited : (11)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.