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Volumn 409, Issue 2, 2003, Pages 689-695

Modeling dissimilar components of the eclipsing binary EK Cep: Does the primary star have a rapidly rotating core?

Author keywords

Binaries: eclipsing; Stars: evolution Stars: abundances; Stars: individual: EK Cep; Stars: interiors; Stars: rotation

Indexed keywords

ASTRONOMY; COSMIC RAYS; SOLAR RADIATION; SPECTRUM ANALYSIS;

EID: 0141993484     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031118     Document Type: Article
Times cited : (20)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.