Interstellar H3(+) - Possible detection of the 1(10)-1(11) transition of H2D

Details Interstellar H3(+) - Possible detection of the 1(10)-1(11) transition of H2D Interstellar H3(+) - Possible detection of the 1(10)-1(11) transition of H2D

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...294l..45p&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 294, July 1, 1985, p. L45-L48.

Astronomy and Astrophysics

Astrophysics

46

Deuterium, Gas-Ion Interactions, Interstellar Chemistry, Interstellar Gas, Molecular Clouds, Abundance, Electron Transitions, Line Spectra, Submillimeter Waves

Scientific paper

An interstellar line has been detected in emission at the expected submillimeter wavelength of the 110→111 transition of H2D+, the deuterated version of the primary ion (H3+) in the favored ion-molecule reaction scheme for interstellar gas phase chemistry. The strength of the line is in approximate agreement with the theoretically anticipated H2D+ abundance.

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