Fragmentation of collapsing clouds and properties of star forming regions in different types of galaxies.

Details Fragmentation of collapsing clouds and properties of star forming regions in different types of galaxies. Fragmentation of collapsing clouds and properties of star forming regions in different types of galaxies.

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6...66i&link_type=abstract

Kinematika Fiz. Nebesn. Tel, Tom 6, No. 1, p. 66 - 72

Computer Science

Collapsing Clouds: Star-Forming Regions, Collapsing Clouds: Fragmentation

Scientific paper

The investigation of the thermal instability in collapsing clouds with initial masses M ≡ 108 - 109Msun and initial temperature T ≍ 104K is carried out. The thermal instability is shown to arise at T ≤ 4000K, when the cooling rate on heavy elements becomes comparable to the cooling rate of the main source, i.e. molecular hydrogen. The star forming region properties for different types of galaxies are discussed.

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