Multimessenger model for the starburst galaxy M82

Elsa De Cea Del Pozo, Diego F. Torres, Ana Y.Rodriguez Marrero

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Resum

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 Cherenkov Telescope Array telescopes are made. The model is also used to self-consistently compute the (all flavors) emission of neutrinos resulting from this starburst galaxy. This can be used in considerations of diffuse contributions of such objects. © 2009. The American Astronomical Society.
Idioma originalAnglès
Pàgines (de-a)1054-1060
RevistaAstrophysical Journal
Volum698
Número2
DOIs
Estat de la publicacióPublicada - 1 de gen. 2009

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