Simulating Anisotropic Thermal Conduction in Supernova Remnants, Implications for the Interstellar Medium

Details Simulating Anisotropic Thermal Conduction in Supernova Remnants, Implications for the Interstellar Medium Simulating Anisotropic Thermal Conduction in Supernova Remnants, Implications for the Interstellar Medium

2007-11-14

arxiv.org/abs/0711.2295v1

Astronomy and Astrophysics

Astrophysics

Scientific paper

10.1111/j.1365-2966.2008.13121.x

We present a large number of two and a half dimensional simulations of supernova remnants expanding into interstellar media having a range of densities, temperatures and magnetic field strengths. The volume of hot gas produced is strongly dependent on the inclusion of thermal conduction and magnetic fields. The four-volumes and three-areas of hot gas have been catalogued and their dependence on interstellar parameters documented. Simulated line widths of radioactive species ejected by supernovae have also been catalogued.

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