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Compact Symmetric Objects (CSOs) are compact (<1 kpc), jetted Active Galactic Nuclei (AGN), whose jet axes are not aligned close to the line of sight, and whose observed emission is not predominantly relativistically boosted towards us. Two…

Compact Symmetric Objects (CSOs) are jetted Active Galactic Nuclei (AGN) with overall projected size <1 kpc. The classification was introduced to distinguish these objects from the majority of compact jetted-AGN in centimeter wavelength…

Compact symmetric objects (CSOs) are radio-emitting active galactic nuclei (AGNs) typically with a double-lobed radio structure confined to within 1 kpc. CSOs represent the earliest evolutionary phase of jetted AGNs. Some of them may…

Astrophysics of Galaxies · Physics 2020-07-07 M. Krezinger , S. Frey , T. An , S. Jaiswal , Y. Zhang

Compact Symmetric Objects (CSOs), young jetted-AGN of overall projected size <1 kpc, are of great interest due to their youth and evolution. The classification was introduced to distinguish between ~95% of powerful compact extragalactic…

We present results of multifrequency polarimetric VLBA observations of 20 compact radio sources. The observations represent the northern and southern extensions of a large survey undertaken to identify Compact Symmetric Objects (CSOs)…

Astrophysics · Physics 2009-11-10 G. B. Taylor , A. B. Peck

Compact Symmetric Objects (CSOs) are small (less than 1 kpc) radio sources which have symmetric double lobes or jets. The dominant theory for the small size of these objects is that they are young radio sources which could grow into larger…

Astrophysics of Galaxies · Physics 2010-11-11 S. E. Tremblay , G. B. Taylor , J. F. Helmboldt , C. D. Fassnacht , R. W. Romani

Compact Symmetric Objects (CSOs) are young radio galaxies whose jet axes lie close to the plane of the sky, and whose appearance is therefore not dominated by relativistic beaming effects. The small linear sizes of CSOs make them valuable…

Astrophysics · Physics 2009-10-31 A. B. Peck , G. B. Taylor , C. D. Fassnacht , A. C. S. Readhead , R. C. Vermeulen

We use a sample of 54 Compact Symmetric Objects (CSOs) to confirm that there are two unrelated CSO classes: an edge-dimmed, low-luminosity class (CSO~1), and an edge-brightened, high-luminosity class (CSO~2). Using blind tests, we show that…

We present multi-frequency Very Long Baseline Array (VLBA) follow-up observations of VLBA Imaging and Polarimetry Survey sources identified as likely compact symmetric objects (CSOs) or super-massive binary black holes (SBBHs). We also…

Astrophysics of Galaxies · Physics 2016-03-23 S. E. Tremblay , G. B. Taylor , A. A. Ortiz , C. D. Tremblay , J. F. Helmboldt , R. W. Romani

Compact symmetric objects (CSOs) trace the earliest phases of radio-galaxy growth; however, robust classification is difficult when radio cores are weak or invisible. We aim to develop and test a Gaia+VLBI approach that utilizes the…

Astrophysics of Galaxies · Physics 2026-01-14 T. An , Y. Zhang , S. Frey , W. A. Baan , A. Wang

Compact symmetric objects (CSOs) are intrinsically compact extragalactic radio sources that are thought to be the progenitors of classical radio galaxies. To date, evolutionary models have mainly focused on the formation and growth of…

Astrophysics of Galaxies · Physics 2025-05-07 M. Orienti , F. D'Ammando , D. Dallacasa , G. Migliori , P. Rossi , G. Bodo

The class of radio sources known as Compact Symmetric Objects (CSOs) is of particular interest in the study of the evolution of radio galaxies. CSOs are thought to be young (probably ~10^4 years), and a very high fraction of them exhibit HI…

Astrophysics · Physics 2009-10-31 A. B. Peck , G. B. Taylor

We present results of multifrequency polarimetric VLBA observations of 34 compact radio sources. The observations are part of a large survey undertaken to identify CSOs Observed in the Northern Sky (COINS). Compact Symmetric Objects (CSOs)…

Astrophysics · Physics 2009-10-31 A. B. Peck , G. B. Taylor

The radio-loud quasar CTD 135 (2234+282, J2236+2828) has been proposed as a candidate compact symmetric object (CSO), based on its symmetric radio structure revealed by multi-frequency very long baseline interferometry (VLBI) imaging…

Astrophysics of Galaxies · Physics 2022-02-08 S. Frey , K. É. Gabányi , T. An

This paper addresses, for the first time, a key aspect of the phenomenology of Compact Symmetric Objects (CSOs) -- the characteristics of their radio spectra. We present a radio-spectrum description of a complete sample of high luminosity…

Double lobe radio sources associated with active galactic nuclei represent one of the longest studied groups in radio astronomy. A particular sub-group of double radio sources comprises the compact symmetric objects (CSOs). CSOs are…

High Energy Astrophysical Phenomena · Physics 2024-01-26 Andrew G. Sullivan , Roger D. Blandford , Mitchell C. Begelman , Mark Birkinshaw , Anthony C. S. Readhead

Compact Symmetric Objects (CSOs) are a distinct category of jetted active galactic nuclei (AGN) whose optical variability characteristics have not been well investigated. We present here the results of our investigation on the optical flux…

Astrophysics of Galaxies · Physics 2025-05-07 Subhashree Swain , Vaidehi S. Paliya , D. J. Saikia , C. S. Stalin , Arya Venugopal , A. K. Bhavya , C. D. Ravikumar

We present pc-scale images of ten Compact Symmetric Objects (CSO) candidates observed with the European VLBI network (EVN). Five radio sources have been observed at 1.6 GHz, and five more at 2.3/8.4 GHz, the latter subsample with the…

Astrophysics · Physics 2009-11-07 Liu Xiang , Carlo Stanghellini , Daniele Dallacasa , Zhang Haiyan

The Compact Symmetric Objects (CSOs) are small (<1 kiloparsec) and powerful extragalactic radio sources showing emission on both sides of an active galactic nucleus and no signs of strong relativistic beaming. They may be young radio…

Cosmology and Nongalactic Astrophysics · Physics 2011-12-20 K. V. Sokolovsky , Y. Y. Kovalev , A. B. Pushkarev , P. Mimica , M. Perucho

Compact symmetric objects (CSOs) are thought to be short-lived radio sources with two lobes of emission that are separated by less than a kpc in projection. However, studies of such systems at high redshift is challenging due to the limited…

Astrophysics of Galaxies · Physics 2025-10-10 J. P. McKean , C. Spingola , D. M. Powell , S. Vegetti
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