Galactic Supernova Remnant G340.6+0.3

Details Galactic Supernova Remnant G340.6+0.3 Galactic Supernova Remnant G340.6+0.3

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cxo..prop.2722g&link_type=abstract

Chandra proposal ID #10500072

Physics

Scientific paper

We propose a 70 ks Chandra observation of SNR G340.6+0.3. This SNR shows distinctive X-ray line structures between N and S shells. Particularly, in the N region, strongly enhanced X-ray lines from highly ionized S, Ar, and Ca suggest ejecta-dominated emission, reminiscent of Cas A. The proposed Chandra observation is essential to reveal the nature of X-ray emission and the origin of this SNR.

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