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 |
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dc.format.mimetype |
application/pdf |
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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 |