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Related papers: An HST Proper-Motion Study of the Large-scale Jet …

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Jets from active galactic nuclei are thought to play a role in the evolution of their host and local environments, but a detailed prescription is limited by the understanding of the jets themselves. Proper motion studies of compact bright…

High Energy Astrophysical Phenomena · Physics 2023-12-21 Agniva Roychowdhury , Eileen T. Meyer , Markos Georganopoulos , Kassidy Kollmann

We present a detailed analysis of the best-quality multi-wavelength data gathered for the large-scale jet in the core-dominated quasar 3C 273. We analyze all the archival observations of the target with the Chandra X-ray Observatory, the…

High Energy Astrophysical Phenomena · Physics 2017-07-26 Volodymyr Marchenko , D. E. Harris , Michal Ostrowski , Lukasz Stawarz , Artem Bohdan , Marek Jamrozy , Bohdan Hnatyk

We report new results from an HST archival program to study proper motions in the optical jet of the nearby radio galaxy M87. Using over 13 years of archival imaging, we reach accuracies below 0.1c in measuring the apparent velocities of…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-16 Eileen T. Meyer , W. B. Sparks , J. A. Biretta , Jay Anderson , Sangmo Tony Sohn , Roeland P. van der Marel , Colin Norman , Masanori Nakamura

We present red and blue images of the jet of the quasar 3C273 obtained with the WFPC2 on the Hubble Space Telescope as well as a new radio map made with the MERLIN array. The images are of significantly better quality than that of previous…

We present Chandra X-ray (0.2-8 keV) and Very Large Array radio (15 and 5 GHz) images of the $\gamma$-ray bright, superluminal quasar 0827+243. The X-ray jet bends sharply--by ~90 deg., presumably amplified by projection effects--5'' from…

Astrophysics · Physics 2009-11-10 Svetlana Jorstad , Alan Marscher

We present the new HST near-infrared polarimetry, broad and narrow-band imaging, and MERLIN 4.5GHz Multi-Frequency Synthesis radio imaging of 3C 293, a unique radio galaxy whose host is an obvious merger remnant, in an exceptionally…

We present results on the compact steep-spectrum quasar 3C 48 from observations with the VLBA, MERLIN and EVN at multiple radio frequencies. In the 1.5-GHz VLBI images, the radio jet is characterized by a series of bright knots. The active…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 T. An , X. Y. Hong , M. J. Hardcastle , D. M. Worrall , T. Venturi , T. J. Pearson , Z. -Q. Shen , W. Zhao , W. X. Feng

Since its discovery in 1963, 3C273 has become one of the most widely studied quasars with investigations spanning the electromagnetic spectrum. While much has been discovered about this historically notable source, its low-frequency…

The relatively intense X-ray emission from large scale (tens to hundreds kpc) jets discovered with Chandra likely implies that jets (at least in powerful quasars) are still relativistic at that distances from the active nucleus. In this…

Astrophysics · Physics 2009-11-07 F. Tavecchio , G. Ghisellini , A. Celotti

We present results from deep (70 ks) Chandra ACIS observations and Hubble Space Telescope ACS F475W observations of two highly optically polarized quasars belonging to the MOJAVE blazar sample, viz., PKS B0106+013 and 1641+399 (3C345).…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 Preeti Kharb , Matthew Lister , Herman Marshall , Brandon Hogan

We present a detailed study of the X-ray, optical and radio emission from the jet, lobes and core of the quasar PKS 2101-490 as revealed by new Chandra, HST and ATCA images. We extract the radio to X-ray spectral energy distributions from…

In this paper we comment on the possibility for intermittent jet activity in quasar 3C 273 on different time-scales. We propose, that striking morphology of the large-scale radio jet in this source, as well as the apparent lack of its…

Astrophysics · Physics 2009-11-10 L. Stawarz

We present measurements of proper motion of the sub-parsec scale jet at 22 GHz in the nearby FR I galaxy 3C 66B. Observations were made using the VLBA at six epochs over four years. A phase-referencing technique was used to improve the…

Astrophysics of Galaxies · Physics 2017-06-21 Hiroshi Sudou , Satoru Iguchi , Guang-Yao Zhao

Relativistic jets are the most energetic manifestation of the active galactic nucleus (AGN) phenomenon. AGN jets are observed from the radio through gamma-rays and carry copious amounts of matter and energy from the sub-parsec central…

We present the first space VLBI observations of 3C~371, carried out at a frequency of 4.8 GHz. The combination of the high resolution provided by the orbiting antenna Highly Advanced Laboratory for Communications and Astronomy (HALCA) and…

Astrophysics · Physics 2009-10-31 Jose-Luis Gomez , Alan P. Marscher

We present that the model of inverse Compton scattering of cosmic microwave background photons (IC/CMB) could well explain the large-scale jet X-ray radiation of 3C 273, and does not violate new Fermi observations. For the individual knots,…

High Energy Astrophysical Phenomena · Physics 2015-02-25 Wen-Po Liu

We present a 16-month sequence of monthly polarimetric 43 GHz VLBA images of the radio galaxy 3C 120. The images probe the inner regions of the radio jet of this relatively nearby superluminal radio galaxy at a linear resolution of 0.07…

We report on the X-ray emission from the radio jet of 3C 17 from Chandra observations and compare the X-ray emission with radio maps from the VLA archive and with the optical-IR archival images from the Hubble Space Telescope. X-ray…

High Energy Astrophysical Phenomena · Physics 2011-02-11 F. Massaro , D. E. Harris , M. Chiaberge , P. Grandi , F. D. Macchetto , S. A. Baum , C. P. O'Dea , A. Capetti

Recent radio emission, polarization, and Faraday rotation maps of the radio jet of the galaxy 3C 303 have shown that one knot of this jet has a {\it galactic}-scale electric current of $\sim 3\times 10^{18}$ Amp\`ere flowing along the jet…

High Energy Astrophysical Phenomena · Physics 2012-03-01 R. V. E. Lovelace , S. Dyda , P. P. Kronberg

The jet of the quasar 3C273 is observed at different spectral bands. This jet has a knot structure. Jet radiation in radio and optical bands are connected with synchrotron mechanism, while the emission mechanism producing the X-rays is…

Astrophysics · Physics 2007-12-11 E. Yu. Bannikova , M. S. Mykhailova
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