Chandra Observation Of The SNR 0104-72.3 In The SMC

Details Chandra Observation Of The SNR 0104-72.3 In The SMC Chandra Observation Of The SNR 0104-72.3 In The SMC

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21442603l&link_type=abstract

American Astronomical Society, AAS Meeting #214, #426.03; Bulletin of the American Astronomical Society, Vol. 41, p.695

Astronomy and Astrophysics

Astronomy

Scientific paper

We report our 110 ks Chandra observation of the supernova remnant 0104-72.3 in the Small Magellanic Cloud. The X-ray morphology shows two prominent lobes in NW and SE surrounded by soft faint emission. While previous X-ray observations suggested a point-like source in the SE region coincident with a candidate Be star, no such source is detected in our Chandra observation. The X-ray spectra of the lobes show overabundant Fe, broadly consistent with shocked stellar ejecta of Type Ia SN. This work was supported in parts by SAO under Chandra grant GO8-9059X.

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