A 330-360 GHz spectral survey of G34.3+0.15 .2. Chemical modelling

Millar, T.J. and Macdonald, G.H. and Gibb, A.G. (1997) A 330-360 GHz spectral survey of G34.3+0.15 .2. Chemical modelling. Astronomy and Astrophysics, 325 (3). pp. 1163-1173. ISSN 0004-6361. (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)

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We describe a detailed depth-and time-dependent model of the molecular cloud associated with the ultracompact H II region G 34.3+0.15. Previous work on observations of NH3 and CS indicates that the molecular cloud has three distinct physical components:- an ultracompact hot core, a compact hot core and an extended halo. We have used the physical parameters derived from these observations as input to our detailed chemical kinetic modelling. The results of the model calculations are discussed with reference to the different chemistries occuring in each component and are compared with abundances derived from our recent spectral line survey of G 34.3+0.15 (Paper I).

Item Type: Article
Uncontrolled keywords: ISM, individual objects, G 34.3+0.15; ISM, molecules; ISM, abundances
Subjects: Q Science
Q Science > QB Astronomy
Divisions: Faculties > Science Technology and Medical Studies > School of Physical Sciences > Centre for Astrophysics and Planetary Sciences
Depositing User: M.A. Ziai
Date Deposited: 21 Sep 2009 14:56
Last Modified: 21 Sep 2009 14:56
Resource URI: https://kar.kent.ac.uk/id/eprint/18189 (The current URI for this page, for reference purposes)
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