Multi-messenger model for the starburst galaxy M82

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics

Scientific paper

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Accepted for publication in The Astrophysical Journal

Scientific paper

10.1088/0004-637X/698/2/1054

In this paper, a consistent model of the multifrequency emission of the starburst galaxy M82, from radio to gamma-rays is presented and discussed. Predictions for observations with Fermi, MAGIC II/VERITAS and CTA telescopes are made. The model is also used to self-consistenty compute the (all flavors) emission of neutrinos resulting from this starburst galaxy, what can be used in considerations of the diffuse contributions of such objects.

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