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Millimeter observations of organic molecules toward high-mass star formation region G34.26+0.15

Li Fu, Guo-Man Lin

Abstract


To investigate the chemical origination of organic molecules CH3OH, CH3OCH3, C2H5OH, CH3OCH, CH3CN, C2H3CN and C2H5CN in the hot core associated with high-mass star formation region G34.26+0.15, Submillimeter Array observations were made with its 230 GHz receiver. The molecular gas distribution has shown that the oxygen- and nitrogen-containing molecules peak at different positions. Comparing the spatial distributions with rotational temperatures and fractional abundances of the observed molecules, we discuss the possible chemical origination of these organic molecules.


Keywords


astrochemistry — molecular processes — line: identification — ISM: abundances

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DOI: http://dx.doi.org/10.1088/1674%E2%80%934527%2F16%2F12%2F182

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Print ISSN: 1674-4527

Online ISSN: 2397-6209