Fig. 3 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. 3.

The multiwavelength photon spectrum of Cas A. The four broken lines are estimates of the fluxes from synchrotron radiation (S), nonthermal bremsstrahlung (NB), inverse Compton scattering of the cosmic microwave background (IC), and the decay of neutral pions (π⁰). See text for details.

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