MacKay, D.D.S. (1995) The chemistry of silicon in hot molecular cores. Astrophysics and Space Science, 224 (1-2). pp. 507-508. ISSN 0004-640X. (doi:10.1007/BF00667928) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:19362)
| The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided. | |
| Official URL: http://dx.doi.org/10.1007/BF00667928 |
Abstract
The gas phase chemistry of hot molecular cores is thought to depend upon the composition of evaporated ice mantle material and its subsequent gas phase reactions. We have modelled the silicon chemistry in these conditions from an SiH4 precursor and find substantial fractional abundances of SiO, H2SiO and HNSi on a timescale of a few 10(4) yr.
| Item Type: | Article |
|---|---|
| DOI/Identification number: | 10.1007/BF00667928 |
| Additional information: | Document Type: Proceedings Paper |
| Subjects: |
Q Science > QB Astronomy Q Science > QC Physics |
| Divisions: |
Divisions > Division of Natural Sciences > Biosciences Divisions > Division of Natural Sciences > Physics and Astronomy |
| Depositing User: | O.O. Odanye |
| Date Deposited: | 04 Jun 2009 13:15 UTC |
| Last Modified: | 16 Nov 2021 09:57 UTC |
| Resource URI: | https://kar.kent.ac.uk/id/eprint/19362 (The current URI for this page, for reference purposes) |
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