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Volumn 652, Issue 2 I, 2006, Pages 1768-1781

The physics of protoplanetesimal dust agglomerates. I. Mechanical properties and relations to primitive bodies in the solar system

Author keywords

Dust, extinction; Methods: laboratory; Planetary systems: formation; Solar system: formation

Indexed keywords


EID: 33845913555     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/508017     Document Type: Article
Times cited : (194)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.