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Volumn 456, Issue 1, 2006, Pages 215-223

The abundances of nitrogen-containing molecules during pre-protostellar collapse

Author keywords

Astrochemistry; ISM: dust, extinction; ISM: molecules; Stars: formation

Indexed keywords

CRYSTAL MICROSTRUCTURE; GRAVITATIONAL EFFECTS; IONIZATION OF GASES; MOLECULAR PHYSICS; NEODYMIUM COMPOUNDS; NITROGEN;

EID: 33748676292     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065375     Document Type: Article
Times cited : (93)

References (37)
  • 30
    • 0003491205 scopus 로고
    • ed. T. J. Millar, & D. A. Williams (Dordrecht: Kluwer)
    • Smith, I. W. M. 1988, in Rate Coefficients in Astrochemistry, ed. T. J. Millar, & D. A. Williams (Dordrecht: Kluwer), 103
    • (1988) Rate Coefficients in Astrochemistry , pp. 103
    • Smith, I.W.M.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.