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相关论文: A radio study of the double-double radio galaxy 3C…

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Winged, or X-shaped, radio sources form a small class of morphologically peculiar extragalactic sources. We present multi-frequency radio observations of two such sources. We derive maximum ages since any re-injection of fresh particles of…

天体物理学 · 物理学 2009-11-07 J. Dennett-Thorpe , P. A. G. Scheuer , R. A. Laing , A. H. Bridle , G. G. Pooley , W. Reich

We present the analysis of VLA and VLBA observations of the radio source 3C 338, associated with the cD galaxy NGC 6166, the central dominant galaxy of the cluster Abell 2199. The VLBA observations were done at 8.4 and 15.4 GHz, while the…

天体物理学 · 物理学 2011-02-11 G. Gentile , C. Rodriguez , G. B. Taylor , G. Giovannini , S. W. Allen , W. M. Lane , N. E. Kassim

X-shaped radio galaxies (XRGs) are characterised by two pairs of misaligned lobes, namely the active lobes hosting radio jets and the wings. None of the formation mechanisms proposed so far can exhaustively reproduce the diverse features…

星系天体物理 · 物理学 2024-10-09 L. Bruno , M. Brienza , A. Zanichelli , M. Gitti , F. Ubertosi , K. Rajpurohit , T. Venturi , D. Dallacasa

A radio source of the Fanaroff--Riley type II with the angular size of 11.3 arc min is identified with an optical galaxy at z=0.229. Thus, the projected linear extent of the radio structure is 3.14 Mpc which makes it the third largest…

天体物理学 · 物理学 2007-05-23 J. Machalski , M. Jamrozy

Using a combination of observations involving the VLA, MERLIN and global VLBI networks we have made a detailed study of the radio continuum and the neutral hydrogen (HI) kinematics and distribution within the central kiloparsec of the radio…

天体物理学 · 物理学 2009-11-10 R. J. Beswick , A. B. Peck , G. B. Taylor , G. Giovannini

We present multi-frequency simultaneous VLBI radio observations of the flat spectrum radio quasar 1633+382 (4C~38.41) as part of the interferometric monitoring of gamma-ray bright active galactic nuclei (iMOGABA) program combined with…

We present deep Very Large Array imaging of 3C~273 in order to determine the diffuse, large scale radio structure of this famous radio-loud quasar. Diffuse extended structure (radio lobes) is detected for the first time in these…

星系天体物理 · 物理学 2016-12-14 Brian Punsly , Preeti Kharb

We aim to test the model proposed to explain the correlation between the flux density at 15 GHz of a stationary component in the parsec-scale jet and the optical continuum emission in the radio galaxy 3C~390.3. In the model, the…

天体物理学 · 物理学 2009-06-23 J. Leon-Tavares , A. P. Lobanov , V. H. Chavushyan , T. G. Arshakian

We report observations of a bright dumb-bell system of galaxies ($z =0.162$) with the upgraded Giant Metrewave Radio Telescope ($u$GMRT), which show that each member of this gravitationally bound pair of galaxies hosts bipolar radio jets…

星系天体物理 · 物理学 2022-05-25 Gopal-Krishna , Ravi Joshi , Dusmanta Patra , Xiaolong Yang , Luis C. Ho , Paul J. Wiita , Amitesh Omar

We present the results of multifrequency observations of two asymmetric, Mpc-scale radio sources with the Giant Metrewave Radio Telescope (GMRT) and the Very Large Array (VLA). The radio luminosity of these two sources, J1211+743 and…

宇宙学与河外天体物理 · 物理学 2015-03-19 A. Pirya , S. Nandi , D. J. Saikia , M. Singh

In this paper, the second in a series investigating FR II radio galaxies at low frequencies, we use LOFAR and VLA observations between 117 and 456 MHz in addition to archival data to determine the dynamics and energetics of two radio…

Radio galaxies are a subclass of active galactic nuclei in which accretion onto the supermassive black hole releases energy via relativistic jets. The jets are not constantly active throughout the life of the host galaxy and alternate…

星系天体物理 · 物理学 2023-08-30 S. Candini , M. Brienza , A. Bonafede , K. Rajpurohit , N. Biava , M. Murgia , F. Loi , R. J. van Weeren , F. Vazza

We report the results of Giant Metrewave Radio Telescope (GMRT) observations of H{\sc i} absorption towards the FRII radio galaxy 3C321 (J1531+2404), which is associated with an active galaxy interacting with a companion. The absorption…

星系天体物理 · 物理学 2012-08-16 Yogesh Chandola , S. K. Sirothia , D. J. Saikia , Neeraj Gupta

Studies of high redshift radio galaxies can shed light on the activity of active galactic nuclei (AGN) in massive elliptical galaxies, and on the assembly and evolution of galaxy clusters in the Universe. J1606+3124 has been tentatively…

星系天体物理 · 物理学 2022-02-02 Tao An , Ailing Wang , Yingkang Zhang , J. N. H. S. Aditya , Xiaoyu Hong , Lang Cui

The N-galaxy 3C99, a Compact Steep-spectrum Source showing a triple asymmetric structure, has been observed with several arrays of radio telescopes at sub-arcsecond resolution. New images from MERLIN, European VLBI Network and the Very Long…

天体物理学 · 物理学 2009-11-07 F. Mantovani , R. Fanti , C. Ferrari , W. Cotton , T. W. B. Muxlow

Feedback by radio-loud active galactic nuclei (AGN) in galaxy groups is not fully understood. Open questions include the duty cycle of the AGN, the spatial extent of the radio lobes, the effect they have on the intragroup medium, and the…

We report the complex radio properties of the radio galaxy NGC 2329 that resides in the centre of the galaxy cluster Abell 569. For this study, we have used archival data from the Very Large Array (VLA) at various resolutions and…

星系天体物理 · 物理学 2021-05-18 Soumyadeep Das , Preeti Kharb , Raffaella Morganti , Sumana Nandi

The powerful high-redshift quasar J2102+6015 (at z=4.575) may provide useful information for studying supermassive black hole growth, galaxy evolution and feedback in the early Universe. The source has so far been imaged with very long…

星系天体物理 · 物理学 2023-03-20 S. Frey , T. An , K. Gabányi , L. Gurvits , M. Krezinger , A. Melnikov , P. Mohan , Z. Paragi , K. Perger , F. Shu , O. Titov , P. de Vicente , Y. Zhang

We present a study of the flux and spectral variability of the two broad-line radio galaxies (BLRGs) 3C 390.3 and 3C 120, observed almost daily with RXTE for nearly two months each in 1996 and 1997, respectively. Our original motivation for…

天体物理学 · 物理学 2009-11-07 M. Gliozzi , R. M. Sambruna , M. Eracleous

Aims. We selected two radio quasars (J1036+1326 and J1353+5725) based on their 1.4-GHz radio structure, which is dominated by a bright central core and a pair of weaker and nearly symmetric lobes at ~10" angular separation. They are…

宇宙学与河外天体物理 · 物理学 2010-12-15 D. Cseh , S. Frey , Z. Paragi , L. I. Gurvits , K. E. Gabanyi