SCOPUS 정보 검색 플랫폼

Volumn 384, Issue 2, 2002, Pages 554-561

The influence of the magnetic field orientation on the angular momentum loss in the pre-main sequence phase: The case of very slowly rotating magnetic Ap stars

(2) Stepien, K a,b Landstreet, J D a

a UNIVERSITY OF WESTERN ONTARIO (Canada)

b UNIVERSITY OF WARSAW (Poland)

Author keywords

Stars: chemically peculiar; Stars: magnetic fields; Stars: pre main sequence; Stars: rotation

Indexed keywords

MAGNETIC FIELD EFFECTS; MAGNETISM; MAGNETIZATION; ROTATION;

ANGULAR MOMENTUM; MAGNETIC STARS;

ASTROPHYSICS;

EID: 0036495298 PISSN: 00046361 EISSN: None Source Type: Journal
DOI: 10.1051/0004-6361:20020053 Document Type: Article

Times cited : (21)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.