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相关论文: Polarization asymmetry in CSS sources: evidence of…

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The compact steep spectrum (CSS) and gigahertz peaked spectrum (GPS) sources are widely believed to be young radiosources, with ages <10^6 yr. If the activity in the nucleus is fuelled by the supply of gas, one might find evidence of this…

天体物理学 · 物理学 2009-11-07 D. J. Saikia , S. Jeyakumar , F. Mantovani , C. J. Salter , R. E. Spencer , P. Thomasson , P. J. Wiita

According to the currently accepted paradigm compact steep spectrum (CSS) sources are precursors of larger/older objects and gigahertz peaked spectrum (GPS) sources may be earlier stages of CSS sources. In this paper we confront this…

天体物理学 · 物理学 2009-11-07 Andrzej Marecki , Ralph E. Spencer , Magdalena Kunert

We have observed the faintest sample of Gigahertz Peaked Spectrum (GPS) and Compact Steep Spectrum (CSS) sources to date, using the Australia Telescope Compact Array. We test the hypothesis that GPS and CSS sources are the youngest radio…

星系天体物理 · 物理学 2016-12-07 J. D. Collier , R. P. Norris , M. D. Filipović , N. F. H. Tothill

Compact steep-spectrum (CSS) and peaked spectrum (PS) radio sources are compact, powerful radio sources. The multi-frequency observational properties and current theories are reviewed with emphasis on developments since the earlier review…

星系天体物理 · 物理学 2021-04-07 Christopher P. O'Dea , D. J. Saikia

Gigahertz Peaked Spectrum (GPS) and Compact Steep Spectrum (CSS) sources are compact radio galaxies (RGs), with jets extending up to 20 kpc and ages <10^3 years. They are considered to evolve to Fanaroff-Riley RGs, but the real scenario to…

GPS and CSS radio sources are the objects of choice to investigate the evolution of young radio-loud AGN. Previous investigations, mainly based on number counts and source size distributions, indicate that GPS/CSS sources decrease…

天体物理学 · 物理学 2009-11-07 I. A. G. Snellen , K. -H. Mack , R. T. Schilizzi , W. Tschager

Global VLBI observations at 5 GHz have been performed to study the source morphology in 10 compact steep-spectrum (CSS) sources selected from the Peacock & Wall catalogue with the aim of finding asymmetric structures produced by the…

宇宙学与河外天体物理 · 物理学 2015-06-15 D. Dallacasa , M. Orienti , C. Fanti , R. Fanti , C. Stanghellini

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 have studied the interrelation of young AGN with their hosts. The objects of study are the young and powerful GPS and CSS radio sources. Due to their small size, GPS and CSS sources are excellent probes of this relation. Furhthermore,…

天体物理学 · 物理学 2007-05-23 A. Labiano , C. P. O'Dea , P. D. Barthel , R. C. Vermeulen

We present radio observations of 19 candidate compact steep-spectrum (CSS) objects selected from a well-defined, complete sample of 52 B2 radio sources of intermediate strength. These observations were made with the VLA A-array at 4.835…

天体物理学 · 物理学 2009-11-07 D. J. Saikia , P. Thomasson , R. E. Spencer , F. Mantovani , C. J. Salter , S. Jeyakumar

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 objects, should represent the young stage in…

高能天体物理现象 · 物理学 2011-11-07 M. Orienti , D. Dallacasa , G. Giovannini , M. Giroletti , F. D'Ammando

Compact Steep Spectrum (CSS) radio sources are active galactic nuclei that have radio jets propagating only on galactic scales, defined as having projected linear sizes (LS) of up to $20\,$kpc. CSS sources are generally hosted by massive…

星系天体物理 · 物理学 2023-05-10 Yjan A. Gordon , Christopher P. O'Dea , Stefi A. Baum , Keith Bechtol , Chetna Duggal , Peter S. Ferguson

The evolution of symmetric extragalactic radio sources can be characterized by four distinct growth stages of the radio luminosity versus size of the source. The interaction of the jet with the ambient medium results in the formation and…

宇宙学与河外天体物理 · 物理学 2012-11-09 Tao An , Willem A. Baan

The polarisation properties of the intrinsically small (< 20 kpc) radio sources are briefly discussed. At centimetric and decimetric wavelengths, substantial polarised emission is often detected in quasars and, at a lower level, in radio…

天体物理学 · 物理学 2007-05-23 D. Dallacasa

As Compact Steep Spectrum radio sources have been shown to be more asymmetrical than larger sources of similar powers, there is a high probability that they interact with an asymmetric medium in the central regions of the host elliptical…

天体物理学 · 物理学 2009-11-10 S. Jeyakumar , Paul J. Wiita , D. J. Saikia , Jagbir S. Hooda

We present the first systematic search for UV signatures from radio source-driven AGN feedback in Compact Steep Spectrum (CSS) radio galaxies. Owing to their characteristic sub-galactic jets (1-20 kpc projected linear sizes), CSS hosts are…

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

We are entering a new era of sensitive, large-area and multi-frequency radio surveys that will allow us to identify Gigahertz-Peaked Spectrum (GPS) and Compact Steep Spectrum (CSS) radio sources over a wide range in radio luminosity and…

星系天体物理 · 物理学 2016-03-16 Elaine M. Sadler

Radio sources with peaked spectra (peaked spectrum sources, PSS) and compact symmetric objects (CSO) are powerful, compact, and presumably young AGNs and therefore particularly suitable to study aspects of the AGN-host connection. We use a…

星系天体物理 · 物理学 2023-11-28 H. Meusinger , M. Mhaskey

We report first X-ray Chandra observations of a sample of seven low luminosity compact (LLC) sources. They belong to a class of young compact steep spectrum (CSS) radio sources. Four of them have been detected, the other three have upper…

宇宙学与河外天体物理 · 物理学 2015-06-18 M. Kunert-Bajraszewska , A. Labiano , A. Siemiginowska , M. Guainazzi
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