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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7558
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dc.contributor.advisorGupta, Nayantara-
dc.contributor.authorPrince, Raj-
dc.date.accessioned2020-10-19T04:41:44Z-
dc.date.available2020-10-19T04:41:44Z-
dc.date.issued2020-01-
dc.identifier.citationPh.D. Thesis, Jawaharlal Nehru University, New Delhi, 2020en_US
dc.identifier.urihttp://hdl.handle.net/2289/7558-
dc.descriptionOpen Accessen_US
dc.description.abstractThis thesis is aimed to study the strong and spectacular flares of blazar. Blazars belong to a class of active galactic nuclei (AGN) with one of the jets pointing towards the observer. Blazars are observed in all wavelengths and show chaotic flux variability during flaring states. The spectral energy distribution of blazar is characterized by two hump kind of structures. The first one peaks in low energy band (IR to soft X-ray), which is well explained by synchrotron mechanism caused by the relativistic electrons in the magnetic field of the jets. The second one peaks in the high energy band (hard X-ray to gamma-ray), which is thought to be the product of inverse Compton scattering of low energy photons with relativistic electrons within the jets or from outside the jets.en_US
dc.language.isoenen_US
dc.publisherRaman Research Institute, Bangalore.en_US
dc.rightsThis thesis is posted here with the permission of the author. Personal use of this material is permitted. Any other use requires prior permission of the author. By choosing to view this document, you agree to all provisions of the copyright laws protecting it.en_US
dc.subject.classificationAstronomy and Astrophysicsen
dc.titleMulti-wavelength Data Analysis and Theoretical Modeling of Blazar Flaresen_US
dc.typeThesisen_US
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