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

被引：109

作者：

Macdonald, GH ^{[1
]}

Gibb, AG ^{[1
]}

Habing, RJ ^{[1
]}

Millar, TJ ^{[1
]}

机构：

[1] UNIV MANCHESTER,INST SCI & TECHNOL,DEPT PHYS,MANCHESTER M60 1QD,LANCS,ENGLAND

来源：

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1996年 / 119卷 / 02期

关键词：

ISM; individual objects; G; 34.3+0.15; molecules; radio lines; line; identification; abundances;

D O I：

10.1051/aas:1996249

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页码：333 / 367

页数：35

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