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

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

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.162..251s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 162, no. 2, Dec. 1989, p. 251-278. Research supported by the Council of Sc

Astronomy and Astrophysics

Astrophysics

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

Scientific paper

An analysis of 356 available literature references was carried out to select 98 polyatomic neutral molecules, molecular ions, and radicals containing three, four, or five atoms of astrophysical significance. The table, in which these molecular entities are arranged according to molecular weight, contains such information as the spectral region, transition levels, and astrophysical objects where the respective molecules were detected, such as the particular comet, meteorite, planet, or star; the sun; interstellar matter; interstellar cloud; molecular cloud; or Galaxy. In addition, 75 new polyatomic molecules containing from three to five atoms of astrophysical significance are listed.

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