An infrared spectroscopic search for the molecular ion H3(+)

Details An infrared spectroscopic search for the molecular ion H3(+) An infrared spectroscopic search for the molecular ion H3(+)

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...342..855g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 342, July 15, 1989, p. 855-859.

Astronomy and Astrophysics

Astrophysics

29

Hydrogen Ions, Infrared Spectroscopy, Interstellar Chemistry, Molecular Ions, Interstellar Matter, Line Spectra, Molecular Clouds, Rotational Spectra, Vibrational Spectra

Scientific paper

The molecular ion H3(+) is thought to play a fundamental role in the
chemistry of the interstellar medium. Here, a search for infrared
vibration-rotation lines of H3(+) at 4 microns toward five obscured
infrared objects is reported. Upper limits corresponding to H3+ column
densities of (4-10) x 10 to the 14th/sq cm are found.

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