Chemistry on interstellar grains and implications for infrared spectroscopy

Details Chemistry on interstellar grains and implications for infrared spectroscopy Chemistry on interstellar grains and implications for infrared spectroscopy

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.290..109m&link_type=abstract

In ESA, Infrared Spectroscopy in Astronomy p 109-114 (SEE N90-19084 11-89)

Astronomy and Astrophysics

Astronomy

2

Chemical Reactions, Cosmic Dust, Infrared Spectroscopy, Interstellar Matter, Millimeter Waves, Particles, Granular Materials, Molecular Clouds, Molecular Structure

Scientific paper

The infrared and millimeter wave observations, suggesting that gas-grain interaction is important in dense clouds, are reviewed. This interaction results in the formation of H2O ice in clouds having low extinction. It is shown that the gas extinction molecular cores enables to study grain surface processes. The detection of large saturated molecules indicates that the surface chemistry may be complex. The way in which the unidentified infrared emission bands can be affected by chemical processes is considered.

Affiliated with

Also associated with

No associations

Rating

Chemistry on interstellar grains and implications for infrared spectroscopy 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 Chemistry on interstellar grains and implications for infrared spectroscopy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chemistry on interstellar grains and implications for infrared spectroscopy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-764742