Chandra Observation of the Magellanic Cloud Supernova Remnant 0454-672 in N9

Details Chandra Observation of the Magellanic Cloud Supernova Remnant 0454-672 in N9 Chandra Observation of the Magellanic Cloud Supernova Remnant 0454-672 in N9

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...20510105s&link_type=abstract

American Astronomical Society Meeting 205, #101.05; Bulletin of the American Astronomical Society, Vol. 36, p.1510

Astronomy and Astrophysics

Astronomy

1

Scientific paper

A Chandra observation has defined the extent of a supernova remnant in the LMC HII region N9. There is good agreement between X-ray and OIII and SII morphology. In X-rays, the central region is bright and emission from the outer shell is weak. The X-ray spectrum is soft and indicates enhanced Fe abundance in the central region which favors a Type IA SN origin.

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