NON-THERMAL EMISSION FROM GALAXY CLUSTERS AND FUTURE OBSERVATIONS WITH THE FERMI GAMMA-RAY TELESCOPE AND LOFAR
FERMI (formely GLAST) and LOFAR will shortly provide crucial information on the non-thermal components (relativistic particles and magnetic eld) in galaxy clusters. After discussing relevant observational facts that already put important constraints on the properties and origin of non-thermal compon...
Αποθηκεύτηκε σε:
| Εκδόθηκε σε: | Revista Mexicana de Astronomía y Astrofísica |
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| Κύριος συγγραφέας: | |
| Μορφή: | Artigo |
| Γλώσσα: | Espanhol |
| Έκδοση: |
Universidad Nacional Autónoma de México
2009
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| Θέματα: | |
| Διαθέσιμο Online: | https://www.redalyc.org/articulo.oa?id=57115743029 |
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