Molecular gas in starburst galaxies: Line intensities and physical conditions

Details Molecular gas in starburst galaxies: Line intensities and physical conditions Molecular gas in starburst galaxies: Line intensities and physical conditions

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995stin...9530569a&link_type=abstract

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Physics

Carbon Monoxide, Cosmic Gases, Far Infrared Radiation, Line Spectra, Molecular Clouds, Molecular Excitation, Molecular Gases, Starburst Galaxies, Carbon 12, Carbon 13, Hydrocyanic Acid

Scientific paper

We present an extended study of molecular excitation for a selection of
starburst galaxies. It extends a study of the (12)CO/(13)CO 1-0
intensity ratio of these galaxies, with an additional goal to
investigate the notion of a two-type molecular medium in the inner
regions of bright IR galaxies.

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