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Related papers: 3C403: a candidate neutrino-emitting radio galaxy

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We present a Hubble Space Telescope image of the FRII radio galaxy 3C 401, obtained at 1.6 microns with the NICMOS camera in which we identify the infrared counterpart of the brightest region of the radio jet. The jet has a complex radio…

We present a multiwavelength study of the nucleus, environment, jets, and hotspots of the nearby FRII radio galaxy 3C 321, using new and archival data from MERLIN, the VLA, Spitzer, HST, and Chandra. An initially collimated radio jet…

Although connections between flaring blazars and some IceCube neutrinos have been established, the dominant sources for the bulk extragalactic neutrino emissions are still unclear and one widely suggested candidate is a population of radio…

High Energy Astrophysical Phenomena · Physics 2025-08-12 Rong-Qing Chen , Neng-Hui Liao , Xiong Jiang , Yi-Zhong Fan

We present new XMM-Newton EPIC observations of the nuclei of the nearby radio galaxies 3C 305, DA 240, and 4C 73.08, and investigate the origin of their nuclear X-ray emission. The nuclei of the three sources appear to have different…

We present an observation of the radio-galaxy 3C401 and the surrounding intracluster medium (ICM) of its host galaxy cluster by the Chandra X-ray Observatory. This luminous radio-galaxy is notable in that it has characteristics intermediate…

Astrophysics · Physics 2009-11-10 Christopher S. Reynolds , Laura W. Brenneman , John T. Stocke

We present results from a 49.4 ks Chandra/ACIS-S observation of the nearby ($z$=0.059) X-shaped FRII radio galaxy 3C~403. This is the first Chandra observation of an X-shaped radio galaxy, and one of the goals of this pioneering study is to…

Astrophysics · Physics 2009-11-10 R. P. Kraft , M. J. Hardcastle , D. M. Worrall , S. S. Murray

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…

Here we want to investigate X-shaped radio galaxy 3C 315, which is a FRII source, but it lies very close to the FRI/FRII borderline. We used publicly available data from Leahy's atlas of double radio-sources and NASA/IPAC Extragalactic…

Astrophysics of Galaxies · Physics 2025-03-11 V. Borka Jovanović , D. Borka , P. Jovanović

We report the first detection of a water megamaser in a radio-loud galaxy, 3C403, and present a follow-up study using the VLA. 3C403 has been observed as a part of a small sample of FRII galaxies with evidence of nuclear obscuration. The…

Astrophysics · Physics 2009-11-10 A. Tarchi , C. Henkel , M. Chiaberge , K. M. Menten , A. Brunthaler , L. Moscadelli

Context: 3C 273, a well-studied active galactic nucleus (AGN), displays characteristics of both jetted-AGN and Seyfert galaxies, making it an excellent source to study the disc-jet connection in AGN. Aims: To investigate the disk-jet…

High Energy Astrophysical Phenomena · Physics 2025-03-12 Ashwani Pandey , Santanu Mondal , Paul J. Wiita

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…

The standard unified scheme of active galactic nuclei requires the presence of high column densities of gas and dust potentially obscuring the central engine. So far, few direct subarcsecond resolution studies of this material have been…

Astrophysics · Physics 2009-11-13 A. Tarchi , A. Brunthaler , C. Henkel , K. M. Menten , J. Braatz , A. Weiss

The ``central engine'' of AGN is thought to be powered by accretion on a central nucleus believed to be a super-massive black hole. The localization and exact mechanism of the energy release in AGN are still not well understood. We present…

The nearby radio galaxy 3C293 is one of a small group of objects where extreme outflows of neutral hydrogen have been detected. However, due to the limited spatial resolution of previous observations, the exact location of the outflow was…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-16 Elizabeth Mahony , Raffaella Morganti , Bjorn Emonts , Tom Oosterloo , Clive Tadhunter

3C 216 has a weak accretion flow luminosity, well below the Seyfert1/QSO dividing line, weak broad emission lines (BELs) and powerful radio lobes. As a consequence of the extreme properties of 3C 216, it is the most convincing example known…

Astrophysics · Physics 2011-02-11 Brian Punsly

Radio galaxies classified as X-shaped/winged, are characterised by two pairs of extended and misaligned lobes, which suggest a rapid realignment of the jet axis, for which a potential cause is still under debate. Here we analyse the complex…

Astrophysics of Galaxies · Physics 2016-11-02 J. Machalski , M. Jamrozy , L. Stawarz , M. Wezgowiec

The origin of astrophysical neutrinos is one of the most debated topics today. Perhaps the most robust evidence of neutrino counterpart comes from supermassive black holes in active galactic nuclei associated with strongly collimated…

High Energy Astrophysical Phenomena · Physics 2023-06-28 Karri I. I. Koljonen , Konstancja Satalecka , Elina J. Lindfors , Ioannis Liodakis

This paper contains an analysis of short Chandra observations of 19 3C sources with redshifts between 0.3 and 0.5 not previously observed in the X-rays. This sample is part of a project to obtain Chandra data for all of the extragalactic…

High Energy Astrophysical Phenomena · Physics 2015-06-15 F. Massaro , D. E. Harris , G. Tremblay , E. Liuzzo , A. Bonafede , A. Paggi

We present a detailed spectral and spatial analysis of the X-ray properties of the compact and unusual radio galaxy 3C 346, combining information from ROSAT and ASCA. The dominant component of X-ray emission (~ 10^44 ergs/s in each of the…

Astrophysics · Physics 2009-10-31 D. M. Worrall , M. Birkinshaw

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…

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