The applications of astrochemistry

Details The applications of astrochemistry The applications of astrochemistry

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990qjras..31..593w&link_type=abstract

Royal Astronomical Society, Quarterly Journal (ISSN 0035-8738), vol. 31, Dec. 1990, p. 593-605.

Astronomy and Astrophysics

Astronomy

3

Cosmochemistry, Interstellar Chemistry, Molecular Clouds, Starburst Galaxies, Stellar Evolution, Abundance, Chemical Reactions, Cosmic Rays, Interstellar Gas, Radiation Distribution

Scientific paper

Astronomical environments whose chemistry does not involve three-body reactions are presented in a table. Since a clear distinction is not considered possible (because three-body reactions may play important initiating roles in the evolution of gas in the outflows from cool stars or in the initial stages of supernovae ejecta), the list is somewhat arbitrary. The characteristics of the different regions are arranged in a quasi-evolutionary sequence. The parameters in the table tend to be only indicative and include the density, temperature, radiation field, cosmic ray flux, elemental abundances, level of ionization, and dynamical information including age and direction of evolution.

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