| Autor: |
Chen, Andrew, Colafrancesco, Sergio, Shafi, Nebiha |
| Předmět: |
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| Zdroj: |
AIP Conference Proceedings; 2017, Vol. 1792 Issue 1, p1-5, 5p, 1 Graph |
| Abstrakt: |
NGC 1068, the brightest and closest Seyfert 2 galaxy, is the brightest of a handful of non-blazar galaxies observed to emit gamma-rays by the Fermi Gamma-ray Space Telescope[1]. We provide arguments for the hypothesis that galactic outflow driven by the active nucleus is the most likely source of both the radio and gamma-ray spectra and compare our results to other possible explanations including starburst activity and blazar-like jet emission. We finally outline a multi-wavelength observing program in progress to test this hypothesis. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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