Attenuation of TeV γ-rays by the starlight photon field of the host galaxy
The absorption of TeV γ-ray photons produced in relativistic jets by surrounding soft photon fields is a long-standing problem of jet physics. In some cases, the most likely emission site close to the central black hole is ruled out because of the high opacity caused by strong optical and infrared p...
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| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
23 November 2016
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2017, Jahrgang: 465, Heft: 3, Pages: 3767-3774 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stw3032 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stw3032
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| Verfasserangaben: | Michael Zacharias, Xuhui Chen and Stefan J. Wagner |
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Attenuation of TeV γ-rays by the starlight photon field of the host galaxy
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