Far-infrared spectroscopy of galaxies: The 158 micron C(+) line

Details Far-infrared spectroscopy of galaxies: The 158 micron C(+) line Far-infrared spectroscopy of galaxies: The 158 micron C(+) line

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984abas.symp..292c&link_type=abstract

In NASA. Ames Research Center Airborne Astron. Symp. p 292-297 (SEE N85-17848 08-89)

Other

Astronomical Spectroscopy, Carbon, Far Infrared Radiation, Galactic Radiation, Galaxies, Interstellar Gas, Carbon Monoxide, Cooling, Excitation, Luminosity, Molecular Clouds, Positive Ions

Scientific paper

The C II 158 micron fine structure line in six gas rich galaxies was
investigated. These data are combined with other measurements of the C
II line (in various galactic sources) and are compared to studies of the
CO J = approaches O rotational line at 2.6 mm, the H I 21 cm line, and
the far infrared continuum emission in the same objects.

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