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Volumn 212, Issue 2-3, 1996, Pages 331-351

Interstellar silicon-nitrogen chemistry. I. The microwave and the infrared signatures of the HSiN, HNSi, HSiNH2, HNSiH2 and HSiNH+ species

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EID: 0030508064     PISSN: 03010104     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0301-0104(96)00216-9     Document Type: Article
Times cited : (18)

References (60)
  • 1
    • 0040139346 scopus 로고
    • B.E. Turner, BAAS 23 (1991) 933.
    • (1991) BAAS , vol.23 , pp. 933
    • Turner, B.E.1
  • 4
    • 0038955158 scopus 로고
    • What species remain to be seen?
    • ed. P.D. Singh IAU
    • B.E. Turner, What species remain to be seen? in: Astrochemistry of cosmic phenomena, ed. P.D. Singh (IAU, 1992), p.181.
    • (1992) Astrochemistry of Cosmic Phenomena , pp. 181
    • Turner, B.E.1
  • 42
    • 0038955152 scopus 로고
    • Ph.D. Thesis, Université d'Orsay, France
    • B. Hanoune, Ph.D. Thesis, Université d'Orsay, France (1994).
    • (1994)
    • Hanoune, B.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.