CO abundances in the Magellanic Clouds

Details CO abundances in the Magellanic Clouds CO abundances in the Magellanic Clouds

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ncimc...8..243b&link_type=abstract

(Convegno Nazionale di Fisica Cosmica, 2nd, L'Aquila, Italy, May 29-June 2, 1984) Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol

Physics

1

Abundance, Carbon Monoxide, Cosmic Rays, Interstellar Chemistry, Magellanic Clouds, Molecular Clouds, Gas Density, Radiative Transfer, Ultraviolet Radiation

Scientific paper

A tentative numerical model of the chemistry of extragalactic molecular clouds is presented. The model is based on recent observations in the Small and Large Magellanic Clouds. An attempt is made to explain the mechanism of transformation of carbon into carbon monoxide. CO column density vs the total column density of hydrogen nuclei is given for the Galaxy, the Large Magellanic Cloud, and the Small Magellanic Cloud, respectively.

Affiliated with

Also associated with

No associations

Rating

CO abundances in the Magellanic Clouds does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with CO abundances in the Magellanic Clouds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CO abundances in the Magellanic Clouds will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1669315