Numerical model for the SNR DEM L316: Simulated X-ray emission
We present a two-component supernova remnant model for the case of Magellanic remnant DEM L316 obtained from two-dimensional, axisymmetric hydrodynamic simulations. We study different scenarios which consider a possible collision between the shells and also the effects of thermal conduction. Synthet...
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| Autores principales: | Toledo-Roy, J.C., Velázquez, P.F., De Colle, F., González, R.F., Reynoso, E.M., Kurtz, S.E., Reyes-Iturbide, J. |
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| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00358711_v395_n1_p351_ToledoRoy |
| Aporte de: |
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