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dc.contributor.authorDiltz, C.
dc.contributor.authorBöttcher, M.
dc.date.accessioned2017-04-07T06:47:12Z
dc.date.available2017-04-07T06:47:12Z
dc.date.issued2016
dc.identifier.citationDiltz, C. & Böttcher, M. 2016. Leptonic and lepto-hadronic modeling of the 2010 November flare from 3C 454.3. Astrophysical journal, 826: Article no 54. [https://doi.org/10.3847/0004-637X/826/1/54]en_US
dc.identifier.issn0004-637X
dc.identifier.issn1538-4357 (Online)
dc.identifier.urihttp://hdl.handle.net/10394/21161
dc.identifier.urihttps://doi.org/10.3847/0004-637X/826/1/54
dc.identifier.urihttp://iopscience.iop.org/article/10.3847/0004-637X/826/1/54
dc.description.abstractIn this study, we use a one-zone leptonic and a lepto-hadronic model to investigate the multi-wavelength emission and prominent flare of the flat spectrum radio quasar 3C 454.3 in 2010 November. We perform a parameter study with both models to obtain broadband fits to the spectral energy distribution (SED) of 3C 454.3. Starting with the baseline parameters obtained from the fits, we then investigate different flaring scenarios for both models to explain an extreme outburst and spectral hardening of 3C 454.3 that occurred in 2010 November. We find that the one-zone lepto-hadronic model can successfully explain both the broadband multi-wavelength SED and light curves in the optical R, Swift X-Ray Telescope, and Fermi γ-ray band passes for 3C 454.3 during quiescence and the peak of the 2010 November flare. We also find that the one-zone leptonic model produces poor fits to the broadband spectra in the X-ray and high-energy γ-ray band passes for the 2010 November flareen_US
dc.language.isoenen_US
dc.publisherAASen_US
dc.subjectGalaxies: activeen_US
dc.subjectGalaxies: jetsen_US
dc.subjectGamma rays: galaxiesen_US
dc.subjectRadiation mechanisms: non-thermalen_US
dc.subjectRelativistic processesen_US
dc.titleLeptonic and lepto-hadronic modeling of the 2010 November flare from 3C 454.3en_US
dc.typeArticleen_US
dc.contributor.researchID24420530 - Böttcher, Markus


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