Polyatomic molecules, molecular ions, and radicals of astrophysical interest. II

Details Polyatomic molecules, molecular ions, and radicals of astrophysical interest. II Polyatomic molecules, molecular ions, and radicals of astrophysical interest. II

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.162..287s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 162, no. 2, Dec. 1989, p. 287-296. Research supported by the Council of Sc

Astronomy and Astrophysics

Astrophysics

1

Cometary Atmospheres, Free Radicals, Interstellar Matter, Molecular Ions, Polyatomic Molecules, Milky Way Galaxy, Molecular Clouds, Solar System

Scientific paper

A critical analysis of the 70 available literature references was carried out to select 37 polyatomic molecules, molecular ions, and radicals containing six, seven, eight, nine, ten, twelve, or thirteen atoms of astrophysical significance. These include C2H4, CH3OH, N2H4, CH3OD, C3H3(+), H3C2N, H2C2NH, HC2NH2, CH3CN, CH3NC, NH2CHO, CH3SN, C4H2, C5H, CH3N2, H3C3H, CH3C2H, CH3CNH(+), CH3CHO, H3C3N, HC5N, C2N5(+), C2H6, C3H3(+), CH3OCHO, CH3C3N, CH3OCH3, CH3CH2OH, C2H5CN, CH3C4H, CH3C4N, HC7N, C2H5C2H, CH3C5N, HC9N, C4N4H4, and HC11N. The compilation, arranged in a tabular form contains such information as the spectral region, transition levels, and astrophysical objects where the respective molecules were detected. In addition, 214 new polyatomic molecules containing six, seven, eight, nine, or ten atoms of astrophysical significance are listed.

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