| dc.contributor.author | Ramadurai, S | |
| dc.contributor.author | Hoyle, F | |
| dc.contributor.author | Wickramasinghe, N. C | |
| dc.date.accessioned | 2007-05-10T09:14:04Z | |
| dc.date.available | 2007-05-10T09:14:04Z | |
| dc.date.issued | 1993 | |
| dc.identifier.citation | BASI, Vol. 21, pp. 663-667 | en |
| dc.identifier.uri | http://hdl.handle.net/2248/1580 | |
| dc.description.abstract | The 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.extent | 497912 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | en | en |
| dc.publisher | Astronomical Society of India | en |
| dc.subject | Solar system | en |
| dc.subject | Meteor | en |
| dc.title | Critique of Fischer-Tropsch type reactions in the solar nebula | en |
| dc.type | Article | en |