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dc.contributor.authorGokus, A.
dc.contributor.authorRichter, S.
dc.contributor.authorSpanier, F.
dc.contributor.authorKreter, M.
dc.contributor.authorKadler, M.
dc.date.accessioned2018-09-26T09:50:51Z
dc.date.available2018-09-26T09:50:51Z
dc.date.issued2018
dc.identifier.citationGokus, A. et al. 2018. Decomposing blazar spectra into lepto‐hadronic emission components. Astronomische Nachrichten / Astronomical notes, 339(5):331-335. [https://doi.org/10.1002/asna.201813500]en_US
dc.identifier.issn0004-6337
dc.identifier.issn1521-3994 (Online)
dc.identifier.urihttp://hdl.handle.net/10394/31115
dc.identifier.urihttps://doi.org/10.1002/asna.201813500
dc.identifier.urihttps://onlinelibrary.wiley.com/doi/10.1002/asna.201813500
dc.description.abstractThe recently reported coincidences between high‐energy neutrino events and major blazar outbursts reinforce the relevance of lepto‐hadronic emission models for blazars. We study the influence of physical parameters on the neutrino output by modeling blazar spectral energy distributions self‐consistently assuming a relativistically propagating acceleration zone surrounded by a larger cooling zone. We find that the gross features of the spectral energy distribution can readily be explained with the model. A rigorous test requires time‐resolved measurements of blazar spectral energy distributions during an outburst and high‐statistics neutrino measurements to discriminate the leptonic and hadronic emission componentsen_US
dc.language.isoenen_US
dc.publisherWileyen_US
dc.subjectAcceleration of particlesen_US
dc.subjectGalaxies: activeen_US
dc.subjectGalaxies: individual (TXS 0506+056)en_US
dc.titleDecomposing blazar spectra into lepto‐hadronic emission componentsen_US
dc.typeArticleen_US
dc.contributor.researchID25433822 - Richter, Stephan
dc.contributor.researchID25161814 - Spanier, Felix Alexander


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