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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…

星系天体物理 · 物理学 2016-10-19 Alla Miroshnichenko

It is currently accepted that intrinsically compact and bright radio sources characterized by a convex spectrum peaking at frequencies ranging from 100 MHz to a few GHz are young objects. Following the evolutionary models, these objects…

宇宙学与河外天体物理 · 物理学 2010-12-02 M. Orienti , D. Dallacasa

The high-frequency integrated spectra of Compact Steep Spectrum (CSS) sources show breaks with a moderate spectral steepening well fitted by continuous injection synchrotron spectra. In lobe-dominated CSS sources the radiative ages deduced…

天体物理学 · 物理学 2009-10-31 M. Murgia , C. Fanti , R. Fanti , L. Gregorini , U. Klein , K. -H. Mack , M. Vigotti

In this paper we discuss the early phase of radio source evolution as represented by Gigahertz Peaked Spectrum (GPS) and Compact Steep Spectrum (CSS) radio sources. Correlations between their spectral peak and angular size strongly suggest…

天体物理学 · 物理学 2009-10-31 Ignas Snellen , Richard Schilizzi

Before we have determined that giant radio structure is typical for steep-spectrum sources detected with Ukrainian T-shaped Radio Telescope of model 2 (UTR-2). To estimate the jet propagation velocity and environment density of giant radio…

星系天体物理 · 物理学 2019-06-05 Alla Miroshnichenko

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

Two frequency observations, mainly at 1.4 and 5 GHz from the VLA, have been used to study spectral variations along the lobes of some nearby low luminosity radio galaxies that constitute a representative sample selected from the B2…

天体物理学 · 物理学 2007-05-23 P. Parma , M. Murgia , R. Morganti , A. Capetti , H. R. de Ruiter , R. Fanti

We present a radio morphological study and spectral analysis for a sample of 13 cD galaxies in rich and poor clusters of galaxies.} Our study is based on new high sensitivity Giant Metrewave Radio Telescope (GMRT) observations at 1.28 GHz,…

天体物理学 · 物理学 2009-11-13 S. Giacintucci , T. Venturi , M. Murgia , D. Dallacasa , R. Athreya , S. Bardelli , P. Mazzotta , D. J. Saikia

Radio galaxies with a projected linear size > 1 Mpc are classified as giant radio sources. According to the current interpretation these are old sources which have evolved in a low-density ambient medium. Since radiative losses are…

宇宙学与河外天体物理 · 物理学 2015-05-18 E. Orrù , M. Murgia , L. Feretti , F. Govoni , G. Giovannini , W. Lane , N. Kassim , R. Paladino

Compact steep spectrum (CSS) and GHz-peaked spectrum (GPS) radio sources represent a large fraction of the extragalactic objects in flux density-limited samples. They are compact, powerful radio sources whose synchrotron peak frequency…

星系天体物理 · 物理学 2016-03-16 M. Orienti

We point out that the remarkable linearity of the ultra-steep radio spectra of high redshift radio galaxies reflects a previously reported general trend for powerful radio galaxies, according to which the spectral curvature is lesser for…

宇宙学与河外天体物理 · 物理学 2015-05-30 Gopal-Krishna , Mukul Mhaskey , A. Mangalam

This paper deals with the spectral ageing study of a representative sample of compact symmetric objects (CSOs) and compact steep spectrum (CSS) sources. Observations reveal a distinctive high-frequency steepening of the radio spectra of…

天体物理学 · 物理学 2009-11-07 Matteo Murgia

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

The evolutionary stage of a powerful radio source originated by an AGN is related to its linear size. In this context, compact symmetric objects (CSOs), which are powerful and intrinsically small (< 1 kpc) radio sources with a convex…

宇宙学与河外天体物理 · 物理学 2010-06-29 M. Orienti , G. Migliori , A. Siemiginowska , A. Celotti

Multifrequency observations with the GMRT and the VLA are used to determine the spectral breaks in consecutive strips along the lobes of a sample of selected giant radio sources (GRSs) in order to estimate their spectral ages. The maximum…

宇宙学与河外天体物理 · 物理学 2009-05-05 C. Konar , D. J. Saikia , M. Jamrozy , J. Machalski

Many of the powerful radio galaxies observed at high redshift are very small, presumably because they are very young. A simple model, which treats the radio source as a bubble expanding into a radially stratified medium, is capable of…

天体物理学 · 物理学 2007-05-23 Mitchell C. Begelman

This paper describes an investigation of the early evolution of extragalactic radio sources using samples of faint and bright Gigahertz Peaked Spectrum (GPS) and Compact Steep Spectrum (CSS) radio galaxies. Correlations found between their…

天体物理学 · 物理学 2009-10-31 Ignas Snellen , Richard Schilizzi , George Miley , Ger de Bruyn , Malcolm Bremer , Huub Rottgering

We compare two temporal properties of classical double radio sources: i) radiative lifetimes of synchrotron-emitting particles and ii) dynamical source ages. We discuss how these can be quite discrepant from one another, rendering use of…

天体物理学 · 物理学 2008-11-26 Katherine Blundell , Steve Rawlings

The cessation of AGN activity in radio galaxies leads to a remnant phase during which jets are no longer sustained, but lobes can be detected for a period of time before they fade away due to radiative and dynamical energy losses. The…

星系天体物理 · 物理学 2022-12-19 Sushant Dutta , Veeresh Singh , C. H. Ishwara Chandra , Yogesh Wadadekar , Abhijit Kayal

Giant radio sources form the linear size extreme of the extra-galactic radio source population. Using the WENSS survey, we have selected a complete sample of these sources. We have investigated the properties of their radio structures. We…

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