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Volumn 199, Issue 2, 2009, Pages 368-377

Empirical models of pressure and density in Saturn's interior: Implications for the helium concentration, its depth dependence, and Saturn's precession rate

Author keywords

Abundances; interior; interiors; Saturn

Indexed keywords


EID: 58649107877     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/j.icarus.2008.10.005     Document Type: Article
Times cited : (41)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.