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Multi-messenger model for the starburst galaxy M82

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.

preprint2009arXivOpen access
Elsa de Cea del PozoDiego F. TorresAna Y. Rodriguez Marrero
astro-ph.GA
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Open access3 authors1 topic
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Elsa de Cea del PozoDiego F. TorresAna Y. Rodriguez Marrero

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