SNR E0102-72: Completing the Picture

Details SNR E0102-72: Completing the Picture SNR E0102-72: Completing the Picture

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1193c&link_type=abstract

Chandra Proposal ID #04500008

Computer Science

Chandra Proposal Id #04500008

Scientific paper

Chandra HETG observations of the SNR E0102-72 in the SMC reveal ejecta velocities of ~1000 km/sec and suggest pregressive ionization due to the reverse shock. These data have allowed us to generate a velocity map of the SNR, a crucial ingredient for creating a model of the 3D structure of the remnant. By observating the SNR at a second roll roughly orthogonal to the first, we will be able to complete this velocity map and refine our 3D model. Further, we will be able to extend our examination of the ionization structure and the radial profile at the reverse shock front.

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