Models of dark clouds and globules

Details Models of dark clouds and globules Models of dark clouds and globules

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kfnt....3...40a&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 3, July-Aug. 1987, p. 40-44. In Russian.

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Astronomical Models, Dark Matter, Globules, Interstellar Matter, Clouds, Isothermal Processes, Pressure Effects, Turbulence Effects

Scientific paper

Isothermal models of globules sustained in equilibrium by turbulent pressure are constructed. The turbulence velocity varies as the inverse of r exp nu where r is the cloud radius. It is shown that the value of the external pressure can be in the range of 10,000-100,000 K/cu cm. The present model can be used to study clouds with masses of less than about 100 solar masses. It is found that models in which nu is close to 0.5 best describe observational data.

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