A Deep Chandra Observation of SMC SNR 0104-72.3

Details A Deep Chandra Observation of SMC SNR 0104-72.3 A Deep Chandra Observation of SMC SNR 0104-72.3

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cxo..prop.2388p&link_type=abstract

Chandra Proposal ID #09500239

Physics

Chandra Proposal Id #09500239

Scientific paper

We propose to observe the supernova remnant (SNR) 0104-72.3 in the Small Magellanic Cloud (SMC). SNR 0104-72.3 is relatively faint and the X-ray images show ~arcsec scale substructure. There is also an X-ray point source within the SNR boundary. Furthermore, the origin of 0104-72.3 has been controversial between Type Ia and II. X-ray characteristics of 0104-72.3 make a deep Chandra ACIS observation the unique tool for the study of this SNR. Our proposed 120 ks ACIS observation would be useful to reveal the origin of 0104-72.3.

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