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Can the Fe K-alpha Line Reliably Predict Supernova Remnant Progenitors?

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Excluding supersoft X-ray sources as progenitors for four Type Ia supernovae in the Large Magellanic Cloud

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Radio emission from interstellar shocks: Young type Ia supernova remnants and the case of N 103B in the Large Magellanic Cloud

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Chandra Imaging of the Outer Accretion Flow onto the Black Hole at the Center of the Perseus Cluster

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Cr-K EMISSION LINE AS A CONSTRAINT ON THE PROGENITOR PROPERTIES OF SUPERNOVA REMNANTS

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