Elsa de Cea del Pozo, Diego F. Torres, Ana Y. Rodriguez Marrero
Published 2009-01-18, updated 2009-04-04Version 2
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.
Comments: Accepted for publication in The Astrophysical Journal
Journal: Astrophys.J.698:1054-1060,2009
IBEX, SWCX and a Consistent Model for the Local ISM
The optical structure of the starburst galaxy M82 - I: Dynamics of the disk and inner-wind
Modelling of the free-free absorption in the starburst galaxy M82 and the Sgr A Complex
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