Skip to main content
Kent Academic Repository

The chemistry of silicon in hot molecular cores

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)

University of Kent Author Information

  • Depositors only (login required):

Total unique views for this document in KAR since July 2020. For more details click on the image.