On Star Formation Rate and Turbulent Dissipation in Galactic Models

Details On Star Formation Rate and Turbulent Dissipation in Galactic Models On Star Formation Rate and Turbulent Dissipation in Galactic Models

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confs..67k&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 67-67"

Physics

Scientific paper

The models of star formation function and of interstellar medium turbulent energy dissipation are proposed. In these models the turbulent energy of the interstellar medium and its structure is taken into account. It is shown that using the expressions proposed is able to explain the observable star formation lag in the Galaxy. The reliability of the star formation and dissipation models to scenario of Galaxy star populations formation is shown.

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