作者: Carles Badenes , Eduardo Bravo , Kazimierz J. Borkowski
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摘要: We propose to use the thermal X-ray emission from young supernova remnants (SNRs) originated in Type Ia supernovae (SNe) extract relevant information concerning explosion mechanism. focus on differences between numerical 1D and 3D calculations, impact that these could have modeling of SNRs. remnant Tycho (SN 1572) as a test case compare with our predictions, discussing observational features allow accept or discard given model.