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Volumn 664, Issue 2 I, 2007, Pages 1253-1263

What is the driving force to form refractory oxide grains? Silicate spectra depend on their formation environment

Author keywords

Astrochemistry; Infrared: general; Methods: laboratory; Plasmas

Indexed keywords


EID: 34547997105     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/519299     Document Type: Article
Times cited : (7)

References (15)
  • 9
    • 84891262004 scopus 로고    scopus 로고
    • Nelson, R., Thiemens, M., Nuth, J., & Donn, B. 1989, LPS Conf., 19, 559 Nuth, J. A., Rietmeijer, F J. M., & Hill, H. G. M. 2002, Meteoritics Planet. Sci., 37, 1579
    • Nelson, R., Thiemens, M., Nuth, J., & Donn, B. 1989, LPS Conf., 19, 559 Nuth, J. A., Rietmeijer, F J. M., & Hill, H. G. M. 2002, Meteoritics Planet. Sci., 37, 1579


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.