Cosmic rays (CRs) propagate in the Milky Way and interact with the interstellar medium and magnetic fields. These interactions produce emissions that span the electromagnetic spectrum, and are an invaluable tool for understanding the intensities and spectra of CRs in distant regions, far beyond those probed by direct CR measurements.
We present updates on the study of CR properties by combining multi-frequency observations of the interstellar emission and latest CR direct measurements with propagation models. Finally, we make prediction for e-ASTROGAM and AMEGO, proposed gamma-ray missions with special focus at the MeV energy range.
Volume 301 -
35th International Cosmic Ray Conference (ICRC2017) -
Session Gamma-Ray Astronomy. GA-galactic
Multi-wavelength Signatures of Cosmic Rays in the Milky Way
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Pre-published on:
August 16, 2017
Published on:
August 03, 2018
Abstract
DOI: https://doi.org/10.22323/1.301.0692
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.