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- W2588990406 abstract "Spatially-resolved X-ray spectroscopic observations over the past several years have led to the discovery of non-thermal X-ray emission arising in the shells of many young Galactic supernova remnants, most notably SN 1006 and Cas A. This emission is thought to be synchrotron emission from electrons shock accelerated to hundreds of TeV, and thus represents strong evidence that cosmic rays are accelerated in SNR shocks. The inferences made using the X-ray observations are corroborated by the detection of TeV γ-rays from three of these remnants. The recent launches of the Chandra and XMM-Newton Observatories provide powerful new probes for regions of shock acceleration in young supernova remnants. The status of the X-ray observations and their implications are reviewed, including some early Chandra results." @default.
- W2588990406 created "2017-02-24" @default.
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- W2588990406 date "2001-01-01" @default.
- W2588990406 modified "2023-09-27" @default.
- W2588990406 title "Evidence for cosmic ray acceleration in supernova remnants from X-ray observations" @default.
- W2588990406 doi "https://doi.org/10.1063/1.1377120" @default.
- W2588990406 hasPublicationYear "2001" @default.
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