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相关论文: Flux evolution and kinematics of superluminal comp…

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The precessing jet-nozzle scenario previously proposed was applied to interpret the VLBI-measured kinematics of five superluminal components (C4,C5,C9,C10 and C22) and their flux density evolution in blazar 3C345. It is shown that in the…

星系天体物理 · 物理学 2022-07-01 S. J. Qian

The kinematic behavior of superluminal components observed at 43 GHz in blazar 3C454.3 were model-fitted with their light curves interpreted in terms of their Doppler-boosting effect. The relation between the flux evolution of superluminal…

高能天体物理现象 · 物理学 2023-06-13 S. J. Qian

Search for Doppler-boosting effect in flux evolution of superluminal components in blazars has been an important subject, which can help clarify their kinematic and emission properties. The kinematics and flux evolution observed at 15GHz…

星系天体物理 · 物理学 2023-06-12 S. J. Qian

The kinematics and flux evolution of the superluminal knots in blazar 3C345 were interpreted in the framework of the precessing jet-nozzle scenario with a precessing common helical trajectory-pattern. We show that the jet in 3C345 precesses…

高能天体物理现象 · 物理学 2024-02-26 S. J. Qian

The precessing jet-nozzle scenario has been applied to interpret the VLBI-kinematics of twenty-seven superluminal components in blazar 3C345 measured during an about 38-yr period. The superluminal knots could be ejected from a double…

星系天体物理 · 物理学 2022-02-07 S. J. Qian

The Doppler factor ($\delta$) is a fundamental quality for the relativistic jets from active galactic nuclei (AGNs). It is also fundamental to assessing the number of the entire population of the jetted AGN at high redshift ($z$), and…

高能天体物理现象 · 物理学 2025-01-28 Dahai Yan , Haiyun Zhang , Jianeng Zhou , Lijuan Dong

We present results on the modelling of the ejection of a superluminal component in the jet of 3C111. We propose that the component is generated by an injection of dense material followed by a decrease in the injection rate of bulk particles…

天体物理学 · 物理学 2009-02-16 M. Perucho , I. Agudo , J. L. Gomez , M. Kadler , E. Ros , Y. Y. Kovalev

We report a change in the trajectory of a well studied jet component of the quasar 3C279. The component changes in apparent projected speed and direction, and we find it to be moving with a Lorentz factor gamma >~ 15 at an initial angle of…

天体物理学 · 物理学 2009-11-07 D. C. Homan , M. L. Lister , K. I. Kellermann , M. H. Cohen , E. Ros , J. A. Zensus , M. Kadler , R. C. Vermeulen

With their jet pointing towards us, blazars are ideal tools to study the physics and structure of extragalactic jets. Their powerful jets are cosmic particle accelerators and are alleged to be one of the production sites of the high-energy…

高能天体物理现象 · 物理学 2025-11-25 Claudia M. Raiteri

Blazars are among the most powerful extragalactic objects, as a sub-class of active galactic nuclei. They launch relativistic jets and their emitted radiation shows strong variability across the entire electro-magnetic spectrum. The…

高能天体物理现象 · 物理学 2015-08-12 C. M. Fromm , L. Fuhrmann , M. Perucho

We try to propose a tentative relativistic jet model for explaining the entire radio-optical phenomena observed in blazar OJ287, which has been observed quasi-periodically with a cycle of about 12yr in its optical light curve. We…

星系天体物理 · 物理学 2018-11-29 Shanjie Qian

We present a possible scenario for the ejection of a superluminal component in the jet of the Broad Line Radio Galaxy 3C111 in early 1996. VLBI observations at 15 GHz discovered the presence of two jet features on scales smaller than one…

天体物理学 · 物理学 2008-09-29 M. Perucho , I. Agudo , J. L. Gomez , M. Kadler , E. Ros , Y. Y. Kovalev

Blazars are a subclass of radio-loud active galactic nuclei (AGNs), where the jet is aligned close to the line of sight. Blazars emission is dominated by non-thermal processes, where Doppler boosted radiation originates from a relativistic…

高能天体物理现象 · 物理学 2021-08-19 Jakub Juryšek , Vitalii Sliusar , Dimitri Moulin , Roland Walter

Blazar emission is dominated by non-thermal radiation from a relativistic jet pointing toward us, therefore undergoing Doppler beaming. This is responsible for flux enhancement and contraction of the variability time scales, so that most…

高能天体物理现象 · 物理学 2019-08-13 C. M. Raiteri , M. Villata

We investigate the relativistic jet of the powerful radio-emitting blazar J1429+5406 at redshift z=3.015. Our understanding of jet kinematics in z>3 quasars is still rather limited, based on a sample of less than about 50 objects. The…

星系天体物理 · 物理学 2025-05-14 Dávid Koller , Sándor Frey

In a two-component jet model, the emissions are the sum of the core and extended emissions: $S^{\rm ob}=S_{\rm core}^{\rm ob}+S_{\rm ext}^{\rm ob}$, with the core emissions, $S_{\rm core}^{\rm ob}= f S_{\rm ext}^{\rm ob}\delta^{q}$, being a…

高能天体物理现象 · 物理学 2017-06-28 Yun-Tian Li , Shao-Yu Fu , Huan-Jian Feng , Si-Le He , Chao Lin , Jun-Hui Fan , Denise Costantin , Yu-Tao Zhang

Recent multi-wavelength observations of 3C454.3, in particular during its giant outburst in 2005, put severe constraints on the location of the 'blazar zone', its dissipative nature, and high energy radiation mechanisms. As the optical,…

天体物理学 · 物理学 2010-11-11 M. Sikora , R. Moderski , G. M. Madejski

Observations of blazar jets are shrouded in relativistic effects, thus hindering our understanding of their intrinsic properties and dominant physical processes responsible for their generation, evolution,radiation and particle emission. In…

高能天体物理现象 · 物理学 2015-06-16 I. Liodakis , V. Pavlidou

The properties of wave-like helically twisted normal mode structures on steady relativistic jets are summarized. Wave speeds are a function of the wavelength and less than the jet speed. However, normal mode interference can lead to both…

天体物理学 · 物理学 2009-10-31 Philip E. Hardee

We present a model for relativistic jets which generates a particular angular distribution of Lorentz factor and energy per solid angle. We consider a fireball with specific internal energy E/M launched with bulk Lorentz factor \gamma_B.…

高能天体物理现象 · 物理学 2015-06-16 Paul C. Duffell , Andrew I. MacFadyen
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