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

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We present new Hubble, Gemini-S, and Chandra observations of the radio galaxy 0313-192, which hosts a 350-kpc double source and jets, even though previous data have suggested that it is a spiral galaxy. We measure the bulge scale and…

天体物理学 · 物理学 2009-11-11 William C. Keel , Raymond E. White , Frazer N. Owen , Michael J. Ledlow

We report the results from a 200 ks Chandra observation of the z=1.786 radio galaxy 3C294 and its cluster environment, increasing by tenfold our earlier observation. The diffuse emission, extending about 100 kpc around the nucleus, has a…

天体物理学 · 物理学 2009-09-17 A. C. Fabian , J. S. Sanders , C. S. Crawford , S. Ettori

We report the discovery of a remnant radio AGN J1615+5452 in the field of ELAIS-N1. GMRT continuum observations at 150, 325 and 610 MHz combined with archival data from the 1.4 GHz NVSS survey were used to derive the radio spectrum of the…

星系天体物理 · 物理学 2020-07-01 Z. Randriamanakoto , C. H. Ishwara-Chandra , A. R. Taylor

We present multi-wavelength monitoring results for the broad-line radio galaxy 3C 120 in the MeV/GeV, sub-millimeter, and 43 GHz bands over six years. Over the past two years, Fermi-LAT sporadically detected 3C 120 with high significance…

高能天体物理现象 · 物理学 2015-06-23 Y. T. Tanaka , A. Doi , Y. Inoue , C. C. Cheung , L. Stawarz , Y. Fukazawa , M. A. Gurwell , M. Tahara , J. Kataoka , R. Itoh

The so-called double-double structure in radio sources is the most conspicuous signature of their restarted activity. Observations indicate that in the majority of double-double radio sources (DDRS), the span of the radio lobes is larger…

宇宙学与河外天体物理 · 物理学 2009-10-28 Andrzej Marecki , Marek Szablewski

PBC J2333.9-2343 is a giant radio galaxy at z = 0.047 with a bright central core associated to a blazar nucleus. If the nuclear blazar jet is a new phase of the jet activity, then the small orientation angle suggest a dramatic change of the…

We present a detailed Fermi/LAT data analysis for the broad-line radio galaxy 3C 120. This source has recently entered into a state of increased gamma-ray activity which manifested itself in two major flares detected by Fermi/LAT in…

高能天体物理现象 · 物理学 2016-03-23 Mateusz Janiak , Marek Sikora , Rafal Moderski

Here we present the spectropolarimetric observations of the radio loud active galaxy 3C 390.3 in the period 2009-2014 (24 epochs). The galaxy has been observed with the 6-meter telescope of SAO RAS using the SCORPIO spectropolarimeter. We…

星系天体物理 · 物理学 2015-06-23 V. L. Afanasiev , A. I. Shapovalova , L. C. Popovic , N. V. Borisov

We report the detection of very broad HI absorption against the central regions of the radio galaxy 3C293. The absorption profile, obtained with the Westerbork Synthesis Radio Telescope, has a full width at zero intensity of about 1400 km/s…

天体物理学 · 物理学 2009-11-10 R. Morganti , T. A. Oosterloo , B. H. C. Emonts , J. M. van der Hulst , C. N. Tadhunter

The millisecond-duration radio flashes known as Fast Radio Bursts (FRBs) represent an enigmatic astrophysical phenomenon. Recently, the sub-arcsecond localization (~ 100mas precision) of FRB121102 using the VLA has led to its unambiguous…

The results of a deep submillimetre observation using SCUBA of the powerful radio galaxy 3C324, at redshift z=1.206, are presented. At 850 microns, emission from the location of the host radio galaxy is marginally detected at the 4.2 sigma…

We present the results of a multi-frequency study of the inversion symmetric radio galaxy NGC326 based on Very Large Array observations at 1.4, 1.6, 4.8, 8.5 and 14.9 GHz. The morphological, spectral and polarization properties of this…

天体物理学 · 物理学 2009-11-07 M. Murgia , P. Parma , H. R. de Ruiter , M. Bondi , R. D. Ekers , R. Fanti , E. B. Fomalont

3C 84 (NGC 1275) is the radio source at the center of the Perseus Cluster and exhibits a bright radio jet. We observed the source with the Global Millimeter VLBI Array (GMVA) between 2008 and 2015, with a typical angular resolution of…

We present: 1) a kinematic and morphological study of the giant Lya nebula associated with the radio galaxy MRC2104-242 (z = 2.49) based on integral field spectroscopic VIMOS data from VLT; 2) a photometric study of the host (proto?) galaxy…

This is the third paper of a series exploring the multi-frequency properties of a sample of eleven nearby low-excitation radio galaxies (LERGs) in the southern sky. We are conducting an extensive study of different galaxy components (stars,…

星系天体物理 · 物理学 2020-10-21 I. Ruffa , R. A. Laing , I. Prandoni , R. Paladino , P. Parma , T. A. Davis , M. Bureau

We present full polarization MeerKAT images of the wide-angle tail, giant radio galaxy J1712$-$2435 at 1.3 GHz with 7.\asec5 resolution and an RMS sensitivity of 8 $\mu$Jy beam$^{-1}$. Due to the angular proximity to the Galactic Center…

星系天体物理 · 物理学 2025-08-01 William Cotton , Gourab Giri , P. J. Agnihotri , D. J. Saikia , K. Thorat , F. Camilo

We present Giant Metrewave Radio Telescope (GMRT) 323 MHz radio continuum observations toward 13 radio-loud quasars at $z>5$, sampling the low-frequency synchrotron emission from these objects. Among the 12 targets successfully observed, we…

星系天体物理 · 物理学 2020-09-16 Yali Shao , Jeff Wagg , Ran Wang , Chris L. Carilli , Dominik A. Riechers , Huib T. Intema , Axel Weiss , Karl M. Menten

We report the discovery of large-scale diffuse radio emission South-East of the galaxy cluster MACS J0520.7-1328, detected through high sensitivity Giant Metrewave Radio Telescope 323 MHz observations. This emission is dominated by an…

We report sub-arcsecond scale radio continuum observations of a field of 35 by 22 arcmin centred in NGC3351 obtained with the Multi-Element Radio Linked Interferometer Network (MERLIN). We found 23 radio sources in this field, 6 of which…

We present the GMRT 235 MHz images of three radio galaxies and 610 MHz images of two sources belonging to a complete sample of cD galaxies in rich and poor galaxy clusters. The analysis of the spectral properties confirms the presence of…

天体物理学 · 物理学 2015-06-24 S. Giacintucci , T. Venturi , S. Bardelli , D. Dallacasa , P. Mazzotta , D. J. Saikia