EVN observations of eleven GHz-Peaked-Spectrum radio sources at 2.3/8.4GHz
arXiv:astro-ph/0501068 · doi:10.1051/0004-6361:20041778
Abstract
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 () in the optically thick regime of their convex spectra. Most of the target sources did not have VLBI images at the time this project started. The aim of the work is to find Compact Symmetric Object (CSO) candidates from the ''bright'' GPS samples. These CSOs play a key role in understanding the very early stage of the evolution of individual radio galaxies. The reason for investigating GPS source samples is that CSO candidates are more frequently found among this class of radio sources. In fact both classes, GPS and CSO, represent a small fraction of the flux limited and flat-spectrum samples like PR+CJ1 (PR: Pearson-Readhead survey, CJ1: the first Caltech--Jodrell Bank survey) and CJF (the Caltech--Jodrell Bank flat spectrum source survey) with a single digit percentage progressively decreasing with decreasing flux density limit. Our results, with at least 3, but possibly more CSO sources detected among a sample of 11, underline the effectiveness of our approach. The three confirmed CSO sources (1133+432, 1824+271, and 2121014) are characterized by a symmetric pair of resolved components, each with steep spectral indices. Five further sources (0144+209, 0554026, 0904+039, 0914+114 and 2322040) can be considered likely CSO candidates. The remaining three sources (0159+839, 0602+780 and 0802+212) are either of core-jet type or dominated by a single component at both frequencies.
11 pages, 22 figures, accepted by A&A
References in corpus (14)
- Sub-milliarcsecond Imaging of Quasars and Active Galactic Nuclei III. Kinematics of Parsec-Scale Radio Jets
- The VLBA Calibrator Survey - VCS1
- A complete sample of GHz-Peaked-Spectrum radio sources and its radio properties
- Proper Motions in Compact Symmetric Objects
- The COINS Sample - VLBA Identifications of Compact Symmetric Objects
- The Presence and Distribution of HI Absorbing Gas in Sub-galactic Sized Radio Sources
- 4C +12.50: A Superluminal Precessing Jet in the Recent Merger System IRAS 13451+1232
- The B3-VLA CSS sample. II: VLBA images at 18 cm
- Bi-Directional Relativistic Jets of the Radio Galaxy 1946+708: Constraints on the Hubble Constant
- Optical spectroscopy of faint gigahertz peaked spectrum sources
- EVN observations of candidate Compact Symmetric Objects
- Automated optical identification of a large complete northern hemisphere sample of flat spectrum radio sources with S_6cm > 200 mJy
- Host Galaxies, Obscuration and Nuclear Structure of Three Nearby Compact Symmetric Objects
- Identifying Compact Symmetric Objects in the Southern Sky
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