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相关论文: Restarting activity in radio galaxies

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This Research Note follows up a Letter in which I posit that J1211+743 is a restarted radio source. This means that its structure, where the jet points to the relic lobe, is only apparently paradoxical. Here, I propose the same scenario and…

宇宙学与河外天体物理 · 物理学 2012-09-20 Andrzej Marecki

J2018-556, an X-shaped FR-I radio galaxy provides a unique opportunity to discuss the formation scenarios for the extended structures seen in this class of radio sources. An understanding of the origin of X-shaped source structures has…

天体物理学 · 物理学 2008-06-24 Lakshmi Saripalli , Ravi Subrahmanyan , Tanmoy Laskar , Anton Koekemoer

Double-lobe radio galaxies in the local Universe have traditionally been found to be hosted in elliptical or lenticular galaxies. We report the discovery of four spiral-host double-lobe radio galaxies (J0836+0532, J1159+5820, J1352+3126 and…

We present radio and optical observations of MG0248+0641, which contains a kiloparsec-scale ring-like structure in one of its radio lobes. The radio observations show a typical core-double morphology: a central core between two lobes, each…

In this paper we discuss the results of a programme of spectral synthesis modelling of a sample of starburst radio galaxies in the context of scenarios for the triggering of the activity and the evolution of the host galaxies. The starburst…

宇宙学与河外天体物理 · 物理学 2015-05-20 C. Tadhunter , J. Holt , R. Gonzalez Delgado , J. Rodriguez Zaurin , M. Villar-Martin , R. Morganti , B. Emonts , C. Ramos Almeida , K. Inskip

We present Very Large Array images of a "Double-Double Radio Galaxy", a class of objects in which two pairs of lobes are aligned either side of the nucleus. In this object, B0925+420, we discover a third pair of lobes, close to the core and…

天体物理学 · 物理学 2009-11-13 C. Brocksopp , C. R. Kaiser , A. P. Schoenmakers , A. G. de Bruyn

We present new VLA, MERLIN and VLBI images for the radio galaxy 3C 338, and the results of the monitoring of its arcsecond core flux density. Present high sensitivity observations allow us to investigate the radio structure of this source…

天体物理学 · 物理学 2009-10-30 G. Giovannini , W. D. Cotton , L. Feretti , L. Lara , T. Venturi

We report new, sensitive observations of two z ~ 3-3.5 FIR-luminous radio galaxies, 6C1909+72 and B3J2330+3927, in 12CO J=1-0 with the Karl Jansky VLA and at 100-500um using Herschel, alongside new and archival 12CO J=4-3 observations from…

The radio structures and optical identifications of a sample of 242 sources classified as double-double radio sources by Proctor (2011) from a morphological study of sources in the FIRST (Faint Images of the Radio Sky at Twenty centimeters)…

宇宙学与河外天体物理 · 物理学 2012-08-16 S. Nandi , D. J. Saikia

We present results of a study of large-scale neutral hydrogen (HI) gas in nearby radio galaxies. We find that the early-type host galaxies of different types of radio sources (compact, FR-I and FR-II) appear to contain fundamentally…

天体物理学 · 物理学 2008-02-01 Bjorn Emonts , Raffaella Morganti , Tom Oosterloo , Jacqueline van Gorkom

Australia Telescope Compact Array (ATCA) images of the giant radio galaxy PKS B1545-321 show a pair of oppositely directed beams emerging from a radio core and ending in bright components that are symmetrically located on either side. These…

天体物理学 · 物理学 2009-11-07 Lakshmi Saripalli , Ravi Subrahmanyan , N. Udaya-Shankar

We announce the discovery of a unique combination of features in a radio source identified with the merger galaxy CGCG 292-057. The radio galaxy both exhibits a highly complex, X-like structure and shows signs of recurrent activity in the…

星系天体物理 · 物理学 2012-07-05 D. Kozieł-Wierzbowska , M. Jamrozy , S. Zola , G. Stachowski , A. Kuźmicz

Radio galaxies dominate the radio sky and are essential to the galaxy evolution puzzle. High-resolution studies of statistical samples of radio galaxies are expected to shed light on the triggering mechanisms of the AGN, alternating between…

星系天体物理 · 物理学 2023-11-22 N. Jurlin , R. Morganti , F. Sweijen , L. K. Morabito , M. Brienza , P. Barthel , G. K. Miley

We present a radio morphological study and spectral analysis for a sample of 13 cD galaxies in rich and poor clusters of galaxies.} Our study is based on new high sensitivity Giant Metrewave Radio Telescope (GMRT) observations at 1.28 GHz,…

天体物理学 · 物理学 2009-11-13 S. Giacintucci , T. Venturi , M. Murgia , D. Dallacasa , R. Athreya , S. Bardelli , P. Mazzotta , D. J. Saikia

The galaxy group NGC6338 is one of the most violent group-group mergers known to date. While the central dominant galaxies rush at each other at 1400km/s along the line of sight, with dramatic gas heating and shock fronts detected, the…

We present deep near-infrared images, taken with Subaru Telescope, of the region around the z=1.08 radio source 3C 356 which show it to be associated with a poor cluster of galaxies. We discuss evidence that this cluster comprises two…

天体物理学 · 物理学 2009-11-07 Chris Simpson , Steve Rawlings

There has been a growing body of evidence to suggest that AGN activity, which is powered by mass accretion on to a supermasive black hole, could be episodic, although the range of time scales involved needs to be explored further. The…

宇宙学与河外天体物理 · 物理学 2010-02-16 D. J. Saikia , M. Jamrozy

We present the results of a comparison between the optical morphologies of a complete sample of 46 southern 2Jy radio galaxies at intermediate redshifts (0.05<z<0.7) and those of two control samples of quiescent early-type galaxies: 55…

宇宙学与河外天体物理 · 物理学 2015-05-30 C. Ramos Almeida , P. S. Bessiere , C. Tadhunter , P. G. Pérez-González , G. Barro , K. J. Inskip , R. Morganti , J. Holt , D. Dicken

New Chandra observations of the giant (0.5 Mpc) radio galaxy 4C23.56 at z = 2.5 show X-rays in a linear structure aligned with its radio emission, but anti-correlated with the detailed radio structure. Consistent with the powerful, high-z…

宇宙学与河外天体物理 · 物理学 2015-05-19 Katherine Blundell , Andy Fabian

We present the discovery of a large scale radio structure associated with IGR J17488--2338, a source recently discovered by \emph{INTEGRAL} and optically identified as a broad line AGN at redshift 0.24. At low frequencies, the source…

高能天体物理现象 · 物理学 2014-05-08 Manuela Molina , L. Bassani , A. Malizia , A. J. Bird , A. Bazzano , P. Ubertini , T. Venturi