Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...155..120t&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 155, no. 1, Jan. 1986, p. 120-128.
Astronomy and Astrophysics
Astrophysics
38
Hydrodynamic Equations, Interstellar Matter, Supernova Remnants, Supernovae, Clouds, Density Distribution, Shock Wave Interaction, Spatial Distribution
Scientific paper
The hydrodynamical events resulting from the interaction of a supernova remnant with a high density condensation - a cloudlet, are investigated by means of high resolution two dimensional hydrodynamical calculations. Spherical and cylindrical cloudlets initially immersed in a constant density medium are considered. The evolution and final fate of the cloudlets is shown to depend not only on their original shape, but also on the distance to the explosion site, i.e., on whether the remnant, prior to the interaction, evolves along its Sedov or its radiative phase. However, none of the performed calculation leads to density enhancements which could clearly be related to the filamentary structure, typical of supernova remnants.
Rozyczka Michal
Tenorio-Tagle Guillermo
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