X-ray Emission Line Measurements of SNR 1E0102.2-7219

Details X-ray Emission Line Measurements of SNR 1E0102.2-7219 X-ray Emission Line Measurements of SNR 1E0102.2-7219

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001tysc.confe.185f&link_type=abstract

Two Years of Science with Chandra, Abstracts from the Symposium held in Washington, DC, 5-7 September, 2001, meeting abstract.

Physics

Supernovae, Supernova Remnants And Isolated Neutron Stars

Scientific paper

The young oxygen-rich supernova remnant 1E0102.2-7219 is the brightest SNR in the Small Magellanic Cloud and the second brightest X-ray source in the SMC. This SNR has been observed with the High Energy Transmission Grating Spectrometer (HETGS) of the Chandra X-ray Observatory. The high resolution X-ray spectrum reveals individual emission lines of oxygen, neon, magnesium, and silicon, with little Fe. We present a systematic analysis of flux measurements for the prominent lines and the plasma diagnostics obtained from ratios of these line fluxes.

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