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Volumn 660, Issue 2 II, 2007, Pages

Planets formed in habitable zones of M dwarf stars probably are deficient in volatiles

Author keywords

Astrobiology; Planetary systems: formation; Planets and satellites: formation

Indexed keywords


EID: 34249873525     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/518121     Document Type: Article
Times cited : (151)

References (31)
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.