Laboratory measurements for the astrophysical identification of MgH

Details Laboratory measurements for the astrophysical identification of MgH Laboratory measurements for the astrophysical identification of MgH

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...359l..65z&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 359, Aug. 20, 1990, p. L65, L66.

Astronomy and Astrophysics

Astrophysics

10

Hydrogen, Infrared Spectrometers, Interstellar Matter, Magnesium, Electron Transitions, Laboratories, Molecular Spectra

Scientific paper

A tunable far-infrared spectrometer has been used to observe the pure
rotational spectrum of MgH in a DC discharge of H2 with magnesium. The
frequencies of the hyperfine components of the N = 1 - 0 transition are
predicted to an estimated accuracy of + or - 350 kHz, which should be
sufficient for the astrophysical identification of this species.

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