A 3D numerical model for Kepler's supernova remnant
We present new 3D numerical simulations for Kepler's supernova remnant. In this work we revisit the possibility that the asymmetric shape of the remnant in X-rays is the product of a Type Ia supernova explosion which occurs inside the wind bubble previously created by an AGB companion star. Due...
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| Autores principales: | Toledo-Roy, J.C., Esquivel, A., Velázquez, P.F., Reynoso, E.M. |
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| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00358711_v442_n1_p229_ToledoRoy |
| Aporte de: |
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