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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1580
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dc.contributor.authorRamadurai, S-
dc.contributor.authorHoyle, F-
dc.contributor.authorWickramasinghe, N. C-
dc.date.accessioned2007-05-10T09:14:04Z-
dc.date.available2007-05-10T09:14:04Z-
dc.date.issued1993-
dc.identifier.citationBASI, Vol. 21, pp. 663-667en
dc.identifier.urihttp://hdl.handle.net/2248/1580-
dc.description.abstractThe paucity of kinetic data for the operation of Fischer-Tropsch Type (FTT) reactions, at the appropriate conditions for the primitive solar nebula, is highlighted. The observed isotopic abundances of D, C-13 and N-15 in the meteoritic kerogen are summarized. These are shown to be against the operation of FTT reactions in the primitive solar nebula.en
dc.format.extent497912 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectSolar systemen
dc.subjectMeteoren
dc.titleCritique of Fischer-Tropsch type reactions in the solar nebulaen
dc.typeArticleen
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