The 3-D Interaction of Shocks with Interstellar Clouds

Details The 3-D Interaction of Shocks with Interstellar Clouds The 3-D Interaction of Shocks with Interstellar Clouds

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...183.8308x&link_type=abstract

American Astronomical Society, 183rd AAS Meeting, #83.08; Bulletin of the American Astronomical Society, Vol. 25, p.1422

Astronomy and Astrophysics

Astronomy

Scientific paper

We are using a 3-D PPM hydrodynamic code to study the interaction between a strong shock and an interstellar cloud. The time evolution of clouds with different geometries is studied using different numerical resolutions. To investigate the mixing and fragmentation of the clouds, the time evolution of a number of total integrated properties of the clouds will be presented. Contact with recent observations of the Cygnus Loop will be made.

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