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High Resolution Spectroscopy of Two Oxygen-Rich SNRs with the Chandra HETG
C. R. Canizares, K. A. Flanagan, D. S. Davis +3
The HETG can be used to obtain spatially resolved spectra of moderately extended sources. We present preliminary results for two well studied, oxygen rich supernova remnants in the…
Ionization and Velocity Structure in the Supernova Remnant E0102-72
K. A. Flanagan, C. R. Canizares, D. S. Davis +4
The High Energy Transmission Grating (HETG) Spectrometer aboard the Chandra X-Ray Observatory was used to observe E0102-72, a ~1000 year old, oxygen rich supernova in the Small Mag…
Ionization Structure and the Reverse Shock in E0102-72
K. A. Flanagan, C. R. Canizares, D. S. Davis +3
The young oxygen-rich supernova remnant E0102-72 in the Small Magellanic Cloud has been observed with the High Energy Transmission Grating Spectrometer of Chandra. The high resolut…
Spectral Line Imaging Observations of 1E0102.2-7219
D. S. Davis, K. A. Flanagan, J. C. Houck +5
E0102-72 is the second brightest X-ray source in the Small Magellanic Cloud and the brightest supernova remnant in the SMC. We observed this SNR for ~140 ksec with the High Energy…