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 .
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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.
|Additional information:||Document Type: Proceedings Paper|
|Subjects:||Q Science > QB Astronomy
Q Science > QC Physics
|Divisions:||Faculties > Science Technology and Medical Studies > School of Biosciences
Faculties > Science Technology and Medical Studies > School of Physical Sciences
|Depositing User:||O.O. Odanye|
|Date Deposited:||04 Jun 2009 13:15|
|Last Modified:||08 May 2012 10:49|
|Resource URI:||http://kar.kent.ac.uk/id/eprint/19362 (The current URI for this page, for reference purposes)|
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