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

G.H. Macdonald; A.G. Gibb; R.J. Habing; TJ Millar

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

G.H. Macdonald, A.G. Gibb, R.J. Habing, TJ Millar

Research output: Contribution to journal › Article › peer-review

Abstract

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.

Original language	English
Pages (from-to)	333-367
Number of pages	35
Journal	Astronomy and Astrophysics Supplement Series
Volume	119
Publication status	Published - 1996

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@article{ced7b7ba4d344bb5b37fed1f3a6d89c0,

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

abstract = "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.",

author = "G.H. Macdonald and A.G. Gibb and R.J. Habing and TJ Millar",

year = "1996",

language = "English",

volume = "119",

pages = "333--367",

journal = "Astronomy and Astrophysics Supplement Series",

issn = "0365-0138",

publisher = "EDP Sciences",

}

TY - JOUR

T1 - A 330-360 GHz spectral survey of G 34.3+0.15 .1. Data and physical analysis

AU - Macdonald, G.H.

AU - Gibb, A.G.

AU - Habing, R.J.

AU - Millar, TJ

PY - 1996

Y1 - 1996

N2 - 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.

AB - 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.

M3 - Article

VL - 119

SP - 333

EP - 367

JO - Astronomy and Astrophysics Supplement Series

JF - Astronomy and Astrophysics Supplement Series

SN - 0365-0138

ER -

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

Abstract

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