Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...176..329r&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 176, no. 2, April 1987, p. 329-337. Research supported by the Polska Akademia
Astronomy and Astrophysics
Astrophysics
33
Hydrodynamics, Interstellar Matter, Molecular Clouds, Supernova Remnants, Condensation, Ejection, Numerical Flow Visualization, Shock Waves, Two Dimensional Models
Scientific paper
Hydrodynamical events resulting from interactions of supernova remnants with dense interstellar cloudlets are investigated by means of high-resolution, two dimensional modelling. Three different evolutionary paths of a cloudlet are identified, all of which eventually lead to its strong deformation and expulsion from the remnant. The main factors determining the fate of a cloudlet are the speed and geometry of transmitted and secondary ("attrition") shocks propagating through it. None of the performed calculations leads to structures which could clearly be related to filaments typical of supernova remnants.
Rozyczka Michal
Tenorio-Tagle Guillermo
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