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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2346
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dc.contributor.authorSaxena, P. P-
dc.contributor.authorBhatnagar, S-
dc.contributor.authorSingh, M-
dc.date.accessioned2008-05-26T10:58:14Z-
dc.date.available2008-05-26T10:58:14Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 2, pp. 67 - 73en
dc.identifier.urihttp://hdl.handle.net/2248/2346-
dc.description.abstractThe production of C(1 D) atoms and their role in the production of (C1, C2, C3, C4) hydrocarbons in Titan's atmosphere are discussed. The reaction between C(1 D) atom and H2 molecule to produce the methylidyne (CH) radical (Okabe, 1978) is suggested as a possible mechanism which provides an additional route to the production of hydrocarbons in Titan's atmosphere.en
dc.format.extent189374 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31...67Sen
dc.subjectChemical reactionsen
dc.subjectC(1 D) atomsen
dc.subjectTitan's atmosphereen
dc.titleOn the production of hydrocarbons in Titan's atmosphereen
dc.typeArticleen
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