SNR RCW 103: Ejecta, Blast Wave, and the Central Compact Object

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Scientific paper

Supernova Remnant (SNR) RCW 103 is a young Type II SNR showing bright X-ray shell and the peculiar central compact object (CCO). While the bright X-ray shell appears to be the shocked stellar winds produced by the massive progenitor, other characteristic features for a young Type II SNR such as metal-rich ejecta and the outer blast wave have not been detected. We propose an 80 ks ACIS observation to search for these features. We will also perform spectral and temporal study of the CCO.

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