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Volumn 583, Issue 2 I, 2003, Pages 878-884

The chemical composition of white dwarfs as a test of convective efficiency during core helium burning

Author keywords

Convection; Nuclear reactions, nucleosynthesis, abundances; Stars: evolution; Stars: interiors; White dwarfs

Indexed keywords


EID: 0038772613     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/345427     Document Type: Article
Times cited : (145)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.