Thermal condensation in a turbulent atomic hydrogen flow

Details Thermal condensation in a turbulent atomic hydrogen flow Thermal condensation in a turbulent atomic hydrogen flow

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sf2a.conf..467h&link_type=abstract

SF2A-2004: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 14-18, 2004. Edited by F. Combes, D. Barret

Astronomy and Astrophysics

Astrophysics

Scientific paper

The interstellar neutral hydrogen is a thermally bistable
medium. The dynamical processes with two coexisting phases involve a large range of spatial (and temporal) scales, that need to be adequately represented in numerical simulations. We have performed 2-d simulations of a converging and turbulent flow. A statistical analysis of the fraction and the properties of the different phases has been carried out and is presented.

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