Results 1 to 10 of about 272 (130)
The Remarkable Predictive Power of Infrared Data of Blazars
Blazars are the brightest and most abundant persistent sources in the extragalactic γ -ray sky. Due to their significance, they are often observed across various energy bands, where the data of which can be used to explore potential correlations between ...
P. Giommi +3 more
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Revealing the Variation Mechanism of ON 231 via the Two-component Shock-in-jet Model
The variation mechanism of blazars is a long-standing unresolved problem. In this work, we present a scenario to explain diverse variation phenomena for ON 231, where the jet emissions are composed of the flaring and the less variable components (most ...
Chi-Zhuo Wang, Yun-Guo Jiang
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Ultraviolet Flux and Spectral Variability Study of Blazars Observed with UVIT/AstroSat
Blazars, the peculiar class of active galactic nuclei, are known to show flux variations across the accessible electromagnetic spectrum. Though they have been studied extensively for their flux variability characteristics across wavelengths, information ...
M. Reshma +7 more
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Multiwavelength analysis of the variability of the blazar 3C 273. [PDF]
Fernandes S +4 more
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Active galactic nuclei (AGNs) can power relativistic jets, which are called blazars when pointed close to our line of sight. Depending on the presence or absence of emission lines in their optical spectra, blazars are categorized into flat spectrum radio
Garima Rajguru +3 more
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Properties and Possible Physical Origins of γ-Ray Emission in Extreme Synchrotron Blazars
Extreme synchrotron blazars, characterized by a first peak in their broadband spectral energy distributions (SEDs) at frequencies exceeding 10 ^17 Hz, often exhibit a second peak beyond 1 TeV.
Ji-Shun Lian +5 more
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Blazars are active galactic nuclei known for their extreme variability, offering unique opportunities to study jet physics and high-energy emission mechanisms.
TianFang Zhang +21 more
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Possible links between BL Lacertae objects and quasars from very long baseline interferometry radio data. [PDF]
Gabuzda DC.
europepmc +1 more source
Constraining the PG 1553+113 Binary Hypothesis: Interpreting Hints of a New, 22 yr Period
PG 1553+113 is a well-known blazar exhibiting evidence of a ∼2.2 yr quasiperiodic oscillation (QPO) in the radio, optical, X-ray, and γ -ray bands. Since QPO mechanisms often predict multiple QPOs, we search for a second QPO in its historical optical ...
S. Adhikari +7 more
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Very High-energy (>50 GeV) Gamma-Ray Flux Variability of Bright Fermi Blazars
Understanding the high-energy emission processes and variability patterns are two of the most challenging research problems associated with relativistic jets.
Vaidehi S. Paliya
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