Astrophysical methods and recent proceeding on the researches of CO rotation lines.

Details Astrophysical methods and recent proceeding on the researches of CO rotation lines. Astrophysical methods and recent proceeding on the researches of CO rotation lines.

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000pabei..18...67c&link_type=abstract

Prog. Astron., Vol. 18, No. 1, p. 67 - 74

Astronomy and Astrophysics

Astrophysics

Carbon Monoxide: Interstellar Molecules, Carbon Monoxide: Infrared Spectra

Scientific paper

CO rotational lines at radio wavelengths reveal the cold universe which is undetectable by optical instruments, the giant molecular clouds - the largest objects in the Galaxy and the important phase of the star forming processes-molecular outflow. CO spectra at the wavelength range of 67 - 186 μm are important probes for detecting the objects of kinetic temperature of several hundred degree, i.e., the envelope of carbon or oxygen rich stars, planetary nebulae, young stellar objects and star forming complexes. The main goal of this paper is giving a review towards astrophysical methods and recent proceeding on the research works which base on observing CO rotational lines.

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