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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7473
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dc.contributor.authorPaliya, Vaidehi S-
dc.contributor.authorDiltz, C-
dc.contributor.authorBottcher, M-
dc.contributor.authorStalin, C. S-
dc.contributor.authorBuckley, D-
dc.date.accessioned2020-11-27T01:24:59Z-
dc.date.available2020-11-27T01:24:59Z-
dc.date.issued2015-03-
dc.identifier.citationASI Conference Series, Vol. 12, pp. 113-114en_US
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/7473-
dc.descriptionOpen Access © Astronomical Society of India http://www.astron-soc.in/bulletin/asics_vol012/pdfs/vaidehi.pdfen_US
dc.description.abstractThe blazar 3C 279 exhibited a giant γ-ray outburst in 2013 December and 2014 April. Apart from the very fast γ-ray flux variability, the spectral nature of the flares were also found to vary significantly between these two flaring events. A prominent curvature in the γ-ray spectrum was noticed in 2014 April flare, on the other hand, the 2013 December displayed an extreme hardening of the spectrum. These observations, thus, put strong constraints on our understanding of the underlying particle acceleration mechanisms.en_US
dc.language.isoenen_US
dc.publisherAstronomical Society of Indiaen_US
dc.subjectGalaxies : activeen_US
dc.subjectQuasars : individualen_US
dc.subject3C 279en_US
dc.subjectGalaxies : jetsen_US
dc.subjectGamma-rays : observationsen_US
dc.titleLepto−Hadronic Origin of γ-ray Outbursts of 3C 279en_US
dc.typeArticleen_US
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