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Cited by 191

The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.

Constraining the location of the emitting region in Fermi blazars through rapid γ-ray variability

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Tavecchio, F., Ghisellini, G., Bonnoli, G., Ghirlanda, G.·2010·Monthly Notices of the Royal Astronomical Society: Letters

Abstract

We consider the 1.5-yr Fermi/Large Area Telescope (LAT) light curves (E>100 MeV) of the flat spectrum radio quasars 3C454.3 and PKS1510−089, which show high activity in this period of time. We characterize the duty cycle of the source by comparing the time spent by the sources at different flux levels. We consider in detail the light curves covering periods of extreme flux. The large number of high-energy photons collected by LAT in these events allows us to find evidence of variability on time-scales of a few hours. We discuss the implications of significant variability on such short time-scales that challenge the scenario recently advanced in which the bulk of the γ-ray luminosity is produced in regions of the jet at large distances (tens of parsec) from the black hole.

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Crossref · 10.1111/j.1745-3933.2010.00867.x

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Metadata

Authors
Tavecchio, F., Ghisellini, G., Bonnoli, G., & Ghirlanda, G.
Venue
Monthly Notices of the Royal Astronomical Society: Letters
Published
2010-06-01
Volume
405
Issue
1
Pages
L94-L98
ISSN
  • 1745-3925 (ISSN-L)
  • 1745-3933
OpenAlex
W1927416654
Cited by
191
References
1
FWCI
12.16
Type
journal article
Language
en
Open access
green

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Tavecchio, F., Ghisellini, G., Bonnoli, G., & Ghirlanda, G. (2010). Constraining the location of the emitting region in Fermi blazars through rapid γ-ray variability. Monthly Notices of the Royal Astronomical Society: Letters. https://doi.org/10.1111/j.1745-3933.2010.00867.x

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