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- W2000774556 abstract "I report here on the analysis and interpretation of a Chandra observation of the supernova remnant Kes 32. Kes 32 is rather weak in X-rays because of a large interstellar absorption, which is found to be ~4 × 1022 cm-2, larger than previously reported. Spectral analysis indicates that the ionization age of this object is very young, with net ~ 4 × 109 cm-3 s and a temperature of kTe ~ 1 keV. The X-ray emission peaks at a smaller radius than in the radio. The low ionization age suggests that Kes 32 is a young remnant. However, a young age is in contradiction to the relatively large apparent size, which indicates an age of several thousand years instead of a few hundred years. This problem is discussed in connection with Kes 32's unknown distance and its possible association with the Norma Galactic arm." @default.
- W2000774556 created "2016-06-24" @default.
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- W2000774556 date "2004-04-01" @default.
- W2000774556 modified "2023-09-26" @default.
- W2000774556 title "Revealing the Obscured Supernova Remnant Kesteven 32 with<i>Chandra</i>" @default.
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- W2000774556 doi "https://doi.org/10.1086/381930" @default.
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