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Related papers: A shrinking Compact Symmetric Object: J11584+2450?

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We study the jet physics of the BL Lac object PKS 2233-148 making use of synergy of observational data sets in the radio and gamma-ray energy domains. The four-epoch multi-frequency (4-43 GHz) VLBA observations focused on the parsec-scale…

High Energy Astrophysical Phenomena · Physics 2018-11-28 A. B. Pushkarev , M. S. Butuzova , Y. Y. Kovalev , T. Hovatta

We present multi-frequency observational results for the Compact Steep-Spectrum (CSS) quasar 3C309.1. The observations were carried out with the VSOP at 1.6 and 4.8GHz and the VLBA at 15.4GHz. The source has a distorted, one-sided radio…

Astrophysics · Physics 2008-11-26 Marcin P. Gawronski , Andrzej J. Kus

We present the kinematics of the parsec-scale jet in 3C 84 from 2003 November to 2022 June observed with the Very Long Baseline Array (VLBA) at 43 GHz. We find that the C3 component, a bright feature at the termination region of the jet…

High Energy Astrophysical Phenomena · Physics 2024-05-16 Minchul Kam , Jeffrey A. Hodgson , Jongho Park , Motoki Kino , Hiroshi Nagai , Sascha Trippe , Alexander Y. Wagner

We present the results of simultaneous VLBA polarisation observations of the BL Lacertae object 0820+225 at 5, 8, and 15 GHz, together with earlier images at 5 GHz. This source has an unusually rich total intensity and polarisation…

Astrophysics · Physics 2009-11-06 D. C. Gabuzda , A. B. Pushkarev , N. N. Garnich

Optical light curves of bright BL Lac objects, in particular those having the SED synchrotron peak at frequencies lower than 10E14 Hz, are characterized by long-term trends with time scales of a few decades. These variations are probabily…

Astrophysics · Physics 2007-05-23 E. Massaro , F. Mantovani

We monitored the superluminal QSO 3C 345 at three epochs during a one-year period in 1995--1996, observing with the VLBA at 22, 15, 8.4, and 5 GHz. We imaged the radio source both in total and in polarized intensity. In the images at 5 and…

Astrophysics · Physics 2009-10-31 E. Ros , J. A. Zensus , A. P. Lobanov

We report multi-epoch Very Long Baseline Interferometric (VLBI) observations of the compact radio lobe in the radio galaxy 3C84 (NGC1275) during 2016 - 2020. The image sequence of 3C84 reveals that the hotspot in the radio lobe showed the…

We present the results of EVN polarization observations of fourteen GHz-Peaked-Spectrum (GPS) radio sources at 5 GHz. These sources were selected from bright GPS source samples and we aimed at finding Compact Symmetric Objects (CSOs). We…

Astrophysics · Physics 2016-08-30 Liu Xiang , Cormac Reynolds , Richard Strom , Daniele Dallacasa

Multifrequency VLBA observations of the final group of ten objects in a sample of FIRST-based compact steep spectrum (CSS) sources are presented. The sample was selected to investigate whether objects of this kind could be relics of…

Astrophysics · Physics 2009-11-13 Magdalena Kunert-Bajraszewska , Andrzej Marecki

We present sub-arcsecond ($\theta\sim0.1^{\prime\prime}$) resolution VLA 1.3 cm continuum and 22.2 GHz H$_2$O maser observations toward 15 compact radio continuum sources with rising spectral index and 8 string-like radio continuum…

Solar and Stellar Astrophysics · Physics 2026-01-19 Tatiana M. Rodriguez , Peter Hofner , Emmanuel Momjian , Esteban D. Araya , Ananay Sethi , Viviana Rosero

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). Based on VLBI continuum surveys…

Astrophysics · Physics 2007-05-23 A. B. Peck , G. B. Taylor

Clues to the physical conditions in radio cores of blazars come from measurements of brightness temperatures as well as effects produced by intrinsic opacity. We study the properties of the ultra compact blazar AO 0235+164 with RadioAstron…

We report the results of a 30 ks Chandra ACIS-S observation of the isolated compact object 1RXS J141256.0+792204 (Calvera). The X-ray spectrum is adequately described by an absorbed neutron star hydrogen atmosphere model with an effective…

High Energy Astrophysical Phenomena · Physics 2015-05-13 Andrew S. H. Shevchuk , Derek B. Fox , Robert E. Rutledge

We address the question of why low-luminosity radio sources with similar flat radio spectra show a range of optical activity. The investigation is based on the spectral energy distributions (SEDs) of objects from the 200 mJy sample. We…

Astrophysics · Physics 2015-06-11 S. Anton , I. W. A. Browne , M. J. M. Marcha , M. Bondi , A. Polatidis

X-ray observations unveiled the existence of enigmatic point-like sources at the centre of young supernova remnants (SNRs). These sources, dubbed Central Compact Objects (CCOs), are thought to be neutron stars formed by the supernova…

Astrophysics · Physics 2009-11-13 R. P. Mignani , S. Zaggia , A. De Luca , R. Perna , N. Bassan , P. A. Caraveo

We report on centimeter VLA and VLBI observations of the giant, low power radio galaxy 1144+35. These observations are sensitive to structures on scales from less than 1 parsec to greater than 1 megaparsec. Diffuse steep spectrum lobes on…

Astrophysics · Physics 2009-10-31 G. Giovannini , G. B. Taylor , E. Arbizzani , M. Bondi , W. D. Cotton , L. Feretti , L. Lara , T. Venturi

We present results of EVN observations of eleven GHz-Peaked-Spectrum (GPS) radio sources at 2.3/8.4 GHz. These sources are from the classical ''bright'' GPS source samples with peak flux densities $>$ 0.2 Jy and spectral indices $\alpha <…

Astrophysics · Physics 2007-05-23 L. Xiang , D. Dallacasa , P. Cassaro , D. Jiang , C. Reynolds

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

We present the results of a program to monitor the structure of the radio emission in 42 $\gamma$-ray bright blazars (31 quasars and 11 BL Lac objects) with the VLBA at 43, 22, and occasionally 15 and 8.4 GHz, over the period from November…

We present the historic light curve of the BL Lac object S5 0716+714, spanning the time interval from 1953 to 2003, built using Asiago archive plates and our recent CCD observations, together with literature data. The source shows an…

Astrophysics · Physics 2008-11-26 R. Nesci , E. Massaro , C. Rossi , S. Sclavi , M. Maesano , F. Montagni