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Using a MeerKAT observation of the galaxy cluster A3562 (a member of the Shapley Supercluster), we have discovered a narrow, long and straight, very faint radio filament, which branches out at a straight angle from the tail of a radio…

宇宙学与河外天体物理 · 物理学 2022-08-03 S. Giacintucci , T. Venturi , M. Markevitch , H. Bourdin , P. Mazzotta , P. Merluzzi , D. Dallacasa , S. Bardelli , S. P. Sikhosana , O. Smirnov , G. Bernardi

We report the results of our radio, optical and infra-red studies of a peculiar radio source 4C~35.06, an extended radio-loud AGN at the center of galaxy cluster Abell 407 ($z=0.047$). The central region of this cluster hosts a remarkably…

We present for the first time a study of peculiar giant radio galaxy (GRG) J223301+131502 using deep multi-frequency radio observations from GMRT (323, 612, and 1300 MHz) and LOFAR (144 MHz) along with optical spectroscopic observations…

We report a serendipitous discovery of a pair of relic lobes separated by 1.86 Mpc and straddling the radio-loud quasar 4C 34.47. The axis connecting them makes an appreciable angle with the axis of its well-known double-lobed radio…

星系天体物理 · 物理学 2014-11-10 Andrzej Marecki , Katarzyna Rusinek

We present multifrequency radio continuum as well as HI observations of the superwind galaxy NGC1482, with both the GMRT and the VLA. This galaxy has a remarkable hourglass-shaped optical emission line outflow as well as bi-polar soft X-ray…

天体物理学 · 物理学 2009-11-10 Ananda Hota , D. J. Saikia

We present optical spectra and high-resolution multi-wavelength radio observations of the compact steep-spectrum radio source MRC B1221-423 (z=0.1706). MRC B1221-423 is a very young (~10^5 yr), powerful radio source which is undergoing a…

宇宙学与河外天体物理 · 物理学 2015-05-18 Helen M. Johnston , Jess W. Broderick , Garret Cotter , Raffaella Morganti , Richard W. Hunstead

Diffuse radio emission in galaxy clusters, such as radio halos, relics, and mini halos, is a key tracer of non-thermal processes, turbulence, and magnetic fields within the intra-cluster medium. However, their low surface brightness, as…

天体物理仪器与方法 · 物理学 2026-02-19 Verlon Etsebeth , Michelle Lochner , Konstantinos Kolokythas , Kenda Knowles , Emma Tolley

We present new arcminute resolution radio images of the low surface brightness radio source PKS B1400-33 that is located in the poor cluster Abell S753. The observations consist of 330 MHz VLA, 843 MHz MOST and 1398 and 2378 MHz ATCA data.…

天体物理学 · 物理学 2009-11-07 R. Subrahmanyan , A. J. Beasley , W. M. Goss , K. Golap , R. W. Hunstead

We investigate the properties of the environment around 20 powerful radio galaxies and quasars at redshifts between 0.45 and 1. Using XMM-Newton and Chandra observations we probe the spatial distribution and the temperature of the cluster…

天体物理学 · 物理学 2009-11-13 Elena Belsole , Diana M. Worrall , Martin J. Hardcastle , Judith H. Croston

Radio galaxies are excellent at tracing large-scale structure due to their high bias. We present new results from the TONS08 radio galaxy redshift survey. We find unequivocal evidence for a huge (at least 80 x 80 x 100 Mpc^3)…

天体物理学 · 物理学 2009-11-07 Kate Brand , Steve Rawlings , Gary J. Hill , Mark Lacy

We present new X-ray (Chandra) and radio (ATCA) observations of the z=0.09 radio galaxy PKS B1416-493, a member of the southern equivalent of the 3CRR sample. We find the source to be embedded in a previously unrecognized bright kT=4.6 keV…

高能天体物理现象 · 物理学 2017-03-22 D. M. Worrall , M. Birkinshaw

Superclusters are the largest objects in the Universe, and they provide a unique opportunity to study how galaxy clusters are born at the junction of the cosmic web as well as the distribution of magnetic fields and relativistic particles…

宇宙学与河外天体物理 · 物理学 2021-11-03 V. Parekh , R. Kincaid , K. Thorat , B. Hugo , S. Sankhyayan , R. Kale , N. Oozeer , O. Smirnov , I. Heywood , S. Makhathini , K. van der Heyden

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

In this paper we present results from a radio-optical study of the galaxy populations of the galaxy clusters Abell 1300 and MACS J1931.8$-$2634, a merger and a relaxed system respectively both located at $z \sim 0.3$, aimed at finding…

A recent Chandra observation of the nearby galaxy cluster Abell 585 has led to the discovery of an extended X-ray jet associated with the high-redshift background quasar B3 0727+409, a luminous radio source at redshift z=2.5. This is one of…

高能天体物理现象 · 物理学 2016-01-13 A. Simionescu , Ł. Stawarz , Y. Ichinohe , C. C. Cheung , M. Jamrozy , A. Siemiginowska , K. Hagino , P. Gandhi , N. Werner

We present the results of a high angular resolution (1.1") and sensitivity (maximum of ~0.1 mJy) radio survey at 1-2 GHz in the Galactic Bulge. This complements the X-ray Chandra Galactic Bulge Survey, and investigates the full radio source…

Context. The two nuclei of the starburst galaxy Arp220 contain multiple compact radio sources previously identified as radio supernovae or supernova remnants. Aims. In order to search for an embedded radio AGN, or other possible exotic…

宇宙学与河外天体物理 · 物理学 2018-02-01 F. Batejat , J. E. Conway , A. Rushton , R. Parra , P. J. Diamond , C. J. Lonsdale , C. J. Lonsdale

We present new, multiwavelength Very Large Array observations of the 3 radio galaxies in the cluster Abell 119: 0053-015, 0053-016 and 3C 29. The first two radio galaxies, which lie close to the cluster center, show a narrow-angle-tailed…

天体物理学 · 物理学 2007-05-23 L. Feretti , D. Dallacasa , F. Govoni , G. Giovannini , G. B. Taylor , U. Klein

A faint new radio source has been detected in the nuclear region of the starburst galaxy M82 using MERLIN radio observations designed to monitor the flux density evolution of the recent bright supernova SN2008iz. This new source was…

宇宙学与河外天体物理 · 物理学 2015-05-18 T. W. B. Muxlow , R. J. Beswick , S. T. Garrington , A. Pedlar , D. M. Fenech , M. K. Argo , J. van Eymeren , M. Ward , A. Zezas , A. Brunthaler