Multimessenger model for the starburst galaxy M82

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

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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 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.
Original languageEnglish
Pages (from-to)1054-1060
JournalAstrophysical Journal
Volume698
Issue number2
DOIs
Publication statusPublished - 1 Jan 2009

Keywords

  • Galaxies: individual (M82)
  • Galaxies: starburst
  • Gamma rays: observations
  • Gamma rays: theory
  • Neutrinos

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    De Cea Del Pozo, E., Torres, D. F., & Marrero, A. Y. R. (2009). Multimessenger model for the starburst galaxy M82. Astrophysical Journal, 698(2), 1054-1060. https://doi.org/10.1088/0004-637X/698/2/1054