330-360GHz spectral lines of G 34.3+0.15. (Macdonald+, 1996)

Details 330-360GHz spectral lines of G 34.3+0.15. (Macdonald+, 1996) 330-360GHz spectral lines of G 34.3+0.15. (Macdonald+, 1996)

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..41190333m&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/119/333. Originally published in: 1996A&AS..119..333M

Other

Interstellar Medium

Scientific paper

A 330-360 GHz spectral survey of the hot molecular core associated with the `cometary' ultracompact H II 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. 70 lines remain unidentified. Chemical abundance and rotation temperature have been determined by rotation diagram analysis for 13 species, and lower limits to abundance found for 38 others. The spectral lines identified are tabulated in Table 1 in the form of observed frequency, line brightness temperature and width, the observing session in which the line was observed, the species, transition and its theoretical frequency (if a positive identification can be made). Any comments are listed in the final column. (1 data file).

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