Chemical Evolution of Interstellar Clouds and Variations of Molecular Abundances

Details Chemical Evolution of Interstellar Clouds and Variations of Molecular Abundances Chemical Evolution of Interstellar Clouds and Variations of Molecular Abundances

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jkas...13....9m&link_type=abstract

Journal of Korean Astronomical Society, vol. 13, no. 1, pp. 9-14

Astronomy and Astrophysics

Astronomy

Scientific paper

The abundances of simple molecules are examined in terms of the time-dependent cloud evolution. The formation and destruction mechanisms of H2CO are reviewed. The average value of the fractional abundance of H2CO is derived to be in the range of 10^-10 to 5*10^-9. This is comparable to the observed values. The expected variations of the molecules formed from or destroyed by CO, CI, and C+ whose abundances depend on the evolutionary state of the cloud are discussed.

Affiliated with

Also associated with

No associations

Rating

Chemical Evolution of Interstellar Clouds and Variations of Molecular Abundances 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 Chemical Evolution of Interstellar Clouds and Variations of Molecular Abundances, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chemical Evolution of Interstellar Clouds and Variations of Molecular Abundances will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-756077