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Related papers: Extragalactic radio source evolution under the dua…

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In order to test the unification scheme for double-lobed radio sources, the far-infrared properties of matched samples of radio-galaxies and radio-loud quasars were studied using ISOPHOT. The quasar data were complemented with nearly…

Astrophysics · Physics 2007-05-23 Ilse M. van Bemmel , Peter D. Barthel , Thijs de Graauw

The tailed radio galaxies that have been called ``Type I'' are not a uniform set. To study their dynamics, we have used the Ledlow-Owen data set, which provides a new sample of 250 radio galaxies in nearby Abell clusters. These sources…

Astrophysics · Physics 2009-10-31 J. Eilek , P. Hardee , T. Markovic , M. Ledlow , F. Owen

The spectral evolution of powerful double radio galaxies (FR II's) is thought to be determined by the acceleration of electrons at the termination shock of the jet, their transport through the bright head region into the lobes and the…

Astrophysics · Physics 2009-11-07 K. Manolakou , J. G. Kirk

We investigate the populations and evolution of normal and active galaxies by extending the infrared source count model of Rowan-Robinson (2001) into the radio. The FIR-radio correlation is used to extend the SEDs to the radio region and it…

Astrophysics · Physics 2009-11-10 A. J. King , M. Rowan-Robinson

The simple unification scheme of powerful radio galaxies and quasars, based entirely on the orientation dependent effects, has been confronted with the observed radio structures for 152 radio galaxies and 173 steep spectrum quasars.…

Astrophysics · Physics 2008-02-03 Krzysztof T. Chyzy , Stanislaw Zieba

Symmetric extragalactic radio sources exhibit a baffling array of features - the remarkable symmetry between the two lobes, the emission in the radio frequency range, well collimated jets, core regions emitting blue and ultraviolet light,…

Astrophysics · Physics 2007-05-23 Manoj Thulasidas

We consider evolution properties of galaxies and quasars with steep radio spectrum at the decametre band from the UTR-2 catalogue. The ratios of source's monochromatic luminosities at the decametre and high-frequency bands display the…

Astrophysics of Galaxies · Physics 2016-10-19 Alla Miroshnichenko

Active galactic nuclei (AGNs) can be divided into two major classes, namely radio-loud and radio-quiet AGNs. A small subset of the radio-loud AGNs is called blazars, which are believed to be unified with Fanaroff-Riley type I and type II…

Astrophysics of Galaxies · Physics 2020-03-11 Zhi-Yuan Pei , Jun-Hui Fan , Denis Bastieri , Jiang-He Yang , Hu-Bing Xiao , W. X. Yang

We present polarisation properties at $1.4\,$GHz of two separate extragalactic source populations: passive quiescent galaxies and luminous quasar-like galaxies. We use data from the {\it Wide-Field Infrared Survey Explorer} data to…

Astrophysics of Galaxies · Physics 2015-06-19 J. K. Banfield , D. H. F. M. Schnitzeler , S. J. George , R. P. Norris , T. H. Jarrett , A. R. Taylor , J. M. Stil

Extended extragalactic radio sources have traditionally been classified into FR I and II types, based on the ratio r of the separation S between the brightest regions on either sides of the host galaxy and the total size T of the radio…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 Yen-Ting Lin , Yue Shen , Michael Strauss , Gordon Richards , Ragnhild Lunnan

This review provides the background and current perspective of some of the striking asymmetries exhibited by extragalactic double-lobed radio sources, paying special attention to the reported interrelationships among some of them. We…

Astrophysics · Physics 2007-05-23 Gopal-Krishna , Paul J. Wiita

We investigate the nature of the point-like optical ``cores'' that have been found in the centres of the host galaxies of a majority of radio galaxies by the Hubble Space Telescope. We examine the evidence that these optical cores are…

Astrophysics · Physics 2009-11-10 P. Kharb , P. Shastri

We present a multiwavelength radio study of a sample of nearby Fanaroff-Riley class II (FRII) radio galaxies, matched with the sample of known X-shaped radio sources in size, morphological properties and redshift, using new Giant Metrewave…

Astrophysics · Physics 2015-05-13 Dharam Vir Lal , Martin J. Hardcastle , Ralph P. Kraft

We have performed a multi-dimensional correlation analysis on the observed properties of a statistically complete core-selected sample of compact radio-loud active galactic nuclei, based on data from the VLBI Space Observing Programme…

Astrophysics · Physics 2009-11-06 M. L. Lister , S. J. Tingay , R. A. Preston

We investigate the role of environment on radio galaxy properties by constructing a sample of large ($\gtrsim100$~kpc), nearby ($z<0.3$) radio sources identified as part of the Radio Galaxy Zoo citizen science project. Our sample consists…

It is argued that the new morphological and spectral information gleaned from the recently published LoFAR Two meter Sky Survey data release 2 (LoTSS-2 at 144 MHz) observations of the cluster Abell 980 (A980), in combination with its…

Astrophysics of Galaxies · Physics 2026-04-23 Gopal-Krishna , Surajit Paul , Sameer Salunkhe , Satish Sonkamble

We present an analytical model for the cosmological evolution of the FRII source population. Based on an earlier model for the intrinsic radio luminosity - linear size evolution of these objects, we construct theoretical source samples. The…

Astrophysics · Physics 2009-10-30 Christian R. Kaiser , Paul Alexander

In classifying the ensemble of powerful extragalactic radio sources, considerable evidence has accumulated that radio galaxies and quasars are orientation-dependent manifestations of the same parent population: massive spheroidal galaxies…

Here we discuss evolution and broad-band emission of compact (< kpc) lobes in young radio sources. We propose a simple dynamical description for these objects, consisting of a relativistic jet propagating into a uniform gaseous medium in…

Astrophysics · Physics 2009-11-13 L. Stawarz , L. Ostorero , M. C. Begelman , R. Moderski , J. Kataoka , S. Wagner

Gamma ray bursts (GRB) occur at random points in the sky at cosmological distances. The spectra evolve through X-ray, optical region to possibly radio frequency. Though there are some models, the origin and time evolution of GRB are not…

Astrophysics · Physics 2007-05-23 Manoj Thulasidas