Interstellar chemistry and submillimetre astronomy

Details Interstellar chemistry and submillimetre astronomy Interstellar chemistry and submillimetre astronomy

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990liaco..29..233m&link_type=abstract

In ESA, From Ground-Based to Space-Borne Sub-mm Astronomy p 233-238 (SEE N91-21986 13-89)

Astronomy and Astrophysics

Astronomy

5

Astronomical Models, Interstellar Chemistry, Interstellar Matter, Molecular Clouds, Oxygen Consumption, Photodissociation, Star Formation, Submillimeter Waves, Metal Hydrides, Molecular Spectra, Protostars, Stellar Winds, Surface Reactions

Scientific paper

Astronomical models of diverse astronomical regions are reviewed. Star forming clouds, photodissociation regions, protostellar winds and shocked gas are considered. The oxygen budget in interstellar clouds and metal hybride formation are studied. The chemistries of particular elements in interstellar regions are commented upon. Astronomical models particularly relevant to present and future submillimeter observations are given particular attention. The need to better understand surface chemistry in determining molecular synthesis in certain regions is stressed.

Affiliated with

Also associated with

No associations

Rating

Interstellar chemistry and submillimetre astronomy 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 Interstellar chemistry and submillimetre astronomy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interstellar chemistry and submillimetre astronomy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1632368