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相关论文: Cosmological evolution of the Fanaroff-Riley type …

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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…

天体物理学 · 物理学 2009-10-30 Christian R. Kaiser , Paul Alexander

[Abridged] Radio galaxies and quasars are among the largest and most powerful single objects known and are believed to have had a significant impact on the evolving Universe and its large scale structure. We explore the intrinsic and…

宇宙学与河外天体物理 · 物理学 2015-06-05 Anna D. Kapińska , Phil Uttley , Christian R. Kaiser

Current wide-area radio surveys are dominated by active galactic nuclei, yet many of these sources have no identified optical counterparts. Here we investigate whether one can constrain the nature and properties of these sources, using…

高能天体物理现象 · 物理学 2015-06-23 Sjoert van Velzen , Heino Falcke , Elmar Koerding

Radio-loud active galactic nuclei (RLAGN) play an important role in the evolution of galaxies through the effects on their environment. The two major morphological classes are core-bright (FRI) and edge-bright (FRII) sources. With the…

In this paper the cosmic evolution of the space density of Fanaroff & Riley Class I (FRI) radio sources is investigated out to z ~ 1, in order to understand the origin of the differences between these and the more powerful FRIIs. High…

天体物理学 · 物理学 2009-11-13 E. E. Rigby , P. N. Best , I. A. G. Snellen

The time evolution of giant lobe-dominated radio galaxies (with projected linear size D>1 Mpc if H_{0}=50 km/s/Mpc and q_{0}=0.5 is analysed on the basis of dynamical evolution of the entire FRII-type population. Two basic physical…

天体物理学 · 物理学 2007-05-23 J. Machalski , K. T. Chyzy , M. Jamrozy

We present the results from the analysis of 26 extragalactic radio sources of type FRII which were observed with the VLA at 5 GHz and around the 1.4 GHz band. The sources were selected to have redshifts in the range $ 0.3<z<1.3$, radio…

天体物理学 · 物理学 2017-08-23 J. A. Goodlet , C. R. Kaiser

A time evolution of giant lobe-dominated radio galaxies (with projected linear size $D>1$ Mpc) is analysed on the basis of dynamical evolution of the entire FRII-type population. Two basic physical parameters, namely the jet power $Q_{0}$…

天体物理学 · 物理学 2007-05-23 J. Machalski , K. T. Chyzy , M. Jamrozy

Extragalactic radio sources appear under different morphologies, the most frequent ones are classified as Fanaroff-Riley type I (FR I), typically with lower luminosities, and Fanaroff-Riley type II, (FR II), typically more luminous. This…

高能天体物理现象 · 物理学 2022-03-23 S. Massaglia , G. Bodo , P. Rossi , A. Capetti , A. Mignone

We estimate ages and physical properties of powerful radio galaxies. An analysis of new multi-wavelength VLA observations of eleven very powerful classical double (FRIIb) radio galaxies with redshifts between 0.4 and 1.3 is presented. We…

天体物理学 · 物理学 2009-11-13 Christopher P. O'Dea , Ruth A. Daly , Preeti Kharb , Kenneth A. Freeman , Stefi A. Baum

I define 3 samples of extragalactic radio sources of type FRII, containing 26 objects in total. The control sample consists of 6C and 7C sources with radio-luminosities of around 10E27 W\Hz at 151 MHz and z~1. The other samples contain 3CRR…

天体物理学 · 物理学 2009-09-29 Julie-Ann Goodlet

Extragalactic radio sources have been classified into two classes, Fanaroff-Riley I and II, which differ in morphology and radio power. Strongly emitting sources belong to the edge-brightened FR II class, and weakly emitting sources to the…

高能天体物理现象 · 物理学 2016-12-07 S. Massaglia , G. Bodo , P. Rossi , S. Capetti , A. Mignone

Radio observations of Fanaroff-Riley class II sources often show correlations between the synchrotron emission and the linear-polarimetric distributions. Magnetic position vectors seem to align with the projected emission of both the radio…

宇宙学与河外天体物理 · 物理学 2015-05-28 Martin Huarte-Espinosa , Martin Krause , Paul Alexander

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…

天体物理学 · 物理学 2015-05-13 Dharam Vir Lal , Martin J. Hardcastle , Ralph P. Kraft

Using a self-similar model for the expansion of cocoons surrounding the jets in powerful extragalactic radio sources (type FRII), we investigate the influence of the properties of the gas surrounding these objects on their evolution. The…

天体物理学 · 物理学 2007-05-23 Christian R. Kaiser , Paul Alexander

The time evolution of `fiducial' radio sources derived from fitting the dynamical model of Kaiser et al. (1997) is compared with the observational data for the `clan' sources found in the sample of giant and normal-size FRII-type sources…

天体物理学 · 物理学 2007-05-23 J. Machalski , K. T. Chyzy , M. Jamrozy

This paper focuses on a comparison of the space densities of FRI and FRII sources at different epochs, with a particular focus on FRI sources. First, we present the concluding steps in constructing the Combined NVSS-FIRST Galaxy catalogue…

宇宙学与河外天体物理 · 物理学 2015-05-18 Melanie A. Gendre , P. N. Best , J. V. Wall

Fanaroff-Riley type IIb (FR IIb) radio galaxies provide a modified standard yardstick that allows constraints to be placed on global cosmological parameters. A sample of 20 FR IIb radio galaxies with redshifts between 0 and 2 are compared…

天体物理学 · 物理学 2010-11-19 Ruth A. Daly , E. J. Guerra

This is the second in a series of papers presenting an analytical model for the evolution of FRII radio sources. In this paper we evaluate the expected radio emission from a radio source incorporating energy loss processes for the…

天体物理学 · 物理学 2015-06-24 Christian R. Kaiser , Jane Dennett-Thorpe , Paul Alexander

Fanaroff-Riley class I (FRI) radio galaxies show centre-brightened emission from disrupted lower power jets, while traditionally more luminous class II (FRIIs), are edge-brightened, with relativistic jets terminating in hotspots. Population…

星系天体物理 · 物理学 2026-05-11 B. Barkus , J. H. Croston , B. Mingo , M. J. Hardcastle , G. Gürkan , V. H. Mahatma
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