The role of molecular hydrogen in the generation of star forming regions and blue compact dwarf galaxies

Details The role of molecular hydrogen in the generation of star forming regions and blue compact dwarf galaxies The role of molecular hydrogen in the generation of star forming regions and blue compact dwarf galaxies

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kfnt....5...69i&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 5, Nov.-Dec. 1989, p. 69-74. In Russian.

Computer Science

Compact Galaxies, Dwarf Galaxies, Galactic Evolution, Hydrogen Clouds, Star Formation, Chemical Composition, Chemical Evolution, Gas Ionization, Molecular Clouds

Scientific paper

The dynamic, thermal, and chemical evolution of gas clouds enriched with heavy elements and having an initial temperature of about 10,000 K is investigated. The universal mechanism of the cloud cooling by molecular hydrogen and of the formation of the cool central part of the star forming region is shown to exist irrespectively of the gas chemical composition. The star forming region parameters are obtained and observational consequences of the developed models are discussed.

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