Expected infrared molecular lines from the galactic centre

Details Expected infrared molecular lines from the galactic centre Expected infrared molecular lines from the galactic centre

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hrgc.conf..267b&link_type=abstract

H II regions and the galactic centre : proceedings of the Eighth ESLAB Symposium, 4-7 June 1974, Frascati, Italy, p. 267-272 (SE

Astronomy and Astrophysics

Astronomy

Galactic Nuclei, Infrared Astronomy, Line Spectra, Molecular Spectra, Clouds, Infrared Detectors, Line Shape

Scientific paper

Expected intensities (at earth) of rotational H2 and HD lines are computed for Sgr A and Sgr B2 clouds. Radio molecular data are used to compute the half-widths of these lines. It is shown that some lines are detectable with present infrared techniques. Their observation will provide the first direct estimate of masses and of the D/H ratio in very dense clouds.

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