Fig. 1 from Evidence of X‐Ray Synchrotron Emission from Electrons Accelerated to 40 TeV in the Supernova Remnant Cassiopeia A

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Evidence of X‐Ray Synchrotron Emission from Electrons Accelerated to 40 TeV in the Supernova Remnant Cassiopeia A

Authors: G. E. Allen, J. W. Keohane, E. V. Gotthelf, R. Petre, K. Jahoda, R. E. Rothschild, R. E. Lingenfelter, W. A. Heindl, D. Marsden, D. E. Gruber, M. R. Pelling, and P. R. Blanco

Allen et al. 1997 The Astrophysical Journal Letters 487 L97.

Provider: AAS Journals

Caption: Fig. 1.

The PCA and HEXTE count spectra of Cas A. The histogram is the broken power‐law model of Table 1. The bottom panel shows the ratio of the data to the histogram. See text for details.

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