Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-05-02
Astronomy and Astrophysics
Astrophysics
To appear in "Young Supernova Remnants" (11th Annual Astrophysics Conference in Maryland), S. S. Holt & U. Hwang (eds), AIP, N
Scientific paper
10.1063/1.1377099
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 Transmission Gratings (HETG) aboard the Chandra X-ray Observatory. The small angular size and high surface brightness make this an excellent target for HETG and we resolve the remnant into individual lines. We observe fluxes from several lines which include O VIII Ly$\alpha$, Ly$\beta$, and O VII along with several lines from Ne X, Ne IX and Mg XII. These line ratios provide powerful constraints on the electron temperature and the ionization age of the remnant.
Allen Glenn E.
Canizares Calude R.
Davis David S.
Dewey Dan
Flanagan Kathryn A.
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