Laboratory detection of the protonated carbon dioxide by submillimeter wave spectroscopy

Details Laboratory detection of the protonated carbon dioxide by submillimeter wave spectroscopy Laboratory detection of the protonated carbon dioxide by submillimeter wave spectroscopy

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...138l..11b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 138, no. 1, Sept. 1984, p. L11, L12. Sponsorship: Centre National de la Recher

Astronomy and Astrophysics

Astrophysics

25

Astronomical Spectroscopy, Carbon Dioxide, Molecular Ions, Radio Spectroscopy, Submillimeter Waves, Environmental Laboratories, Interstellar Gas, Line Spectra, Proton Impact, Space Environment Simulation

Scientific paper

Six lines corresponding to the K = 0 and K = 2 components of the J = 15-16 and 16-17 transitions of HCO2(+) have been observed in the laboratory by discharging a mixture of H2 + CO2 + Ar. These lines have been fitted together with the astrophysical lines attributed to HCO2(+) or HOCN, and the B and C constants as well as centrifugal distorsion constants have been determined. This gives a definitive confirmation of the attribution of these astrophysical lines to the protonated carbon dioxide.

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