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- W2078646064 abstract "Using the Position Sensitive Proportional Counter on ROSAT, we detected soft X-ray emission from SN 1986J in NGC 891 approximately nine years after the supernova event. The X-ray emission is characterized by L(x) (0.1-2.5 keV) = 1.6-7 x 10 exp 40 ergs/s, T(x) = 1.0-3.9 keV, and an absorbing column of 5-14 x 10 exp 21/sq cm. The X-ray luminosity, temperature, and absorption column are reproduced surprisingly well in a model where a reverse shock propagates into the outer layers of the exploded star. The large absorbing column is probably intrinsic to the supernova and represents the cooled gas created by a radiative reverse shock." @default.
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- W2078646064 date "1992-10-01" @default.
- W2078646064 modified "2023-09-28" @default.
- W2078646064 title "X-ray emission from SN 1986J in NGC 891" @default.
- W2078646064 doi "https://doi.org/10.1086/186588" @default.
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