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Quasi Periodic Oscillations in Blazars

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dc.contributor.author Gupta, A. C.
dc.date.accessioned 2015-06-03T06:12:28Z
dc.date.available 2015-06-03T06:12:28Z
dc.date.issued 2014-09
dc.identifier.uri http://hdl.handle.net/123456789/1080
dc.description.abstract Here we report our recent discoveries of Quasi-Periodic Oscillations (QPOs) in blazars time series data in X-ray and optical elec- tromagnetic bands. Any such detection can give important clues of the location and nature of the processes of emission mechanism. In the case of radio-quiet AGN, the detected QPOs are very likely to be associated with the accretion disk. But in the case of blazars, it may be associated with jets in the high and outburst states, and in the low-state, it is prob- ably associated with the accretion disk. In this brief review, I summarize the recent QPO detections in blazars. There is one strong evidence of QPO detection in XMM–Newton time series data of narrow line Seyfert 1 galaxy RE J1034 + 396 about which we will also discuss briefly. en_US
dc.language.iso en_US en_US
dc.publisher Indian Academy of Sciences en_US
dc.relation.ispartofseries jaa35-307
dc.subject Galaxies: active—galaxies: quasars: blazars: blazar: individual: 3C 273, S5 0716 + 714, PKS 2155−304, ON 231, AO 0235 + 164, 1ES 2321 + 419. en_US
dc.title Quasi Periodic Oscillations in Blazars en_US
dc.type Article en_US


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