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- W1516033403 abstract "Several physical mechanisms have been studied in order to explain why composite supernova remnants (SNRs) have shell-like morphologies in radio continuum while their X-ray emission is centrally peaked. One of the proposed mechanisms has been the presence of thermal conduction, which can raise the density at the center of SNRs, increasing the X-ray emission from these regions. In this work, we have carried out axisymmetric numerical simulations with the adaptive grid yguazu-a code, including the advection of the magnetic field and the thermal conduction. We have considered cases with anisotropic thermal conduction, as well as with no conduction. We have simulated X-ray emission maps from our numerical simulations for these both cases, and we then compare these predictions with recent X-ray observations of SNRs." @default.
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- W1516033403 date "2003-01-01" @default.
- W1516033403 modified "2023-10-03" @default.
- W1516033403 title "Effects of Anisotropic Thermal Conduction on X-Ray Emission from SNRS" @default.
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