A 330-360 GHz spectral survey of G 34.3+0.15 .1. Data and physical analysis

Macdonald, G.H. and Gibb, A.G. and Habing, R.J. and Millar, T.J. (1996) A 330-360 GHz spectral survey of G 34.3+0.15 .1. Data and physical analysis. Astronomy & Astrophysics Supplement Series, 119 (2). pp. 333-367. ISSN 0365-0138. (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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A 330--360 GHz spectral survey of the hot molecular core associated with the 'cometary' ultracompact HII region G 34.3+/-0.15 observed with the James Clerk Maxwell Telescope has detected 338 spectral lines from at least 35 distinct chemical species plus 19 isotopomers. 70 lines remain unidentified. Chemical abundance and rotation temperature have been determined by rotation diagram analysis for 12 species, and lower limits to abundance found for 38 others.

Item Type: Article
Uncontrolled keywords: ISM, individual objects, G 34.3+0.15; ISM, molecules; radio lines, ISM; line, identification; ISM, abundances
Subjects: Q Science > QB Astronomy
Divisions: Faculties > Science Technology and Medical Studies > School of Engineering and Digital Arts
Depositing User: F.D. Zabet
Date Deposited: 27 Jun 2009 11:13
Last Modified: 27 Jun 2009 11:13
Resource URI: https://kar.kent.ac.uk/id/eprint/18655 (The current URI for this page, for reference purposes)
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