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 original | Anglès |
|---|---|
| Pàgines (de-a) | 1054-1060 |
| Revista | Astrophysical Journal |
| Volum | 698 |
| Número | 2 |
| DOIs | |
| Estat de la publicació | Publicada - 1 de gen. 2009 |
Fingerprint
Navegar pels temes de recerca de 'Multimessenger model for the starburst galaxy M82'. Junts formen un fingerprint únic.Com citar-ho
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver