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- W3020973219 abstract "Abstract We report on the detection of X-ray emission from the supernova remnant (SNR) G359.1-0.5 in a deep ROSAT PSPC pointed observation. The diffuse emission is well confined within the radio shell of the SNR. Its spectrum can be represented by a thermal plasma model at T ~ 1 keV and F x ~ 2×10 −11 erg cm −2 s −1 (0.1–2.0 keV) modified by the column absorption of NH ~ 3 × 10 22 cm −2 . This result supports the view that the source is at a large distance consistent with that from radio observation, and helps to resolve a puzzle about the SNR in previous observations." @default.
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- W3020973219 title "X-ray Emission from G359.1-0.5" @default.
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- W3020973219 doi "https://doi.org/10.1017/s0252921100071359" @default.
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