Multi-messenger model for the starburst galaxy M82
Astrophysics of Galaxies
2011-02-11 v2
Abstract
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.
Cite
@article{arxiv.0901.2688,
title = {Multi-messenger model for the starburst galaxy M82},
author = {Elsa de Cea del Pozo and Diego F. Torres and Ana Y. Rodriguez Marrero},
journal= {arXiv preprint arXiv:0901.2688},
year = {2011}
}
Comments
Accepted for publication in The Astrophysical Journal