VLBI observations of nineteen GHz-Peaked-Spectrum radio sources at 1.6 GHz

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dc.creatorLiu, Xiang
dc.creatorCui, Lang
dc.creatorLuo, Wen-Feng
dc.creatorShi, Wei-Zhao
dc.creatorSong, Hua-Gang
dc.date2007-04-03
dc.date.accessioned2026-07-07T08:14:27Z
dc.date.available2026-07-07T08:14:27Z
dc.descriptionAims and Methods: We present the results of VLBI observations of nineteen GHz-Peaked-Spectrum (GPS) radio sources at 1.6 GHz. Of them, 15 sources are selected from the Parkes Half Jansky (PHJ) sample (Snellen 2002), 4 others are from our previous observation list. We aimed at imaging the structure of GPS sources, searching for Compact Symmetric Objects (CSOs) and studying the absorption for the convex radio spectra of GPS sources. Results: We obtained total intensity 1.6 GHz VLBI images of 17 sources for the first time. Of them, 80% show mini-double-lobe radio structure, indicating that they are CSOs or candidates, and their host AGNs could be edge-on to us. This result suggests that there is a high incidence of mini double-lobe sources (or CSOs) in the PHJ sample. The sources J0323+0534, J1135-0021, J1352+0232, J2058+0540, J2123-0112 and J2325-0344 with measured redshift, showing double-lobe structure with sizes of <1 kpc, are classified as CSOs. Three sources J1057+0012, J1600-0037 and J1753+2750 are considered as core-jet sources according to their morphologies and flux variability.
dc.description11 pages, 12 figures, to appear in AA
dc.identifierhttps://arxiv.org/abs/0704.0310
dc.identifierhttp://arxiv.org/abs/0704.0310
dc.identifierA&A 470, 97-104 (2007)
dc.identifierdoi:10.1051/0004-6361:20077265
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/133128
dc.subjectAstrophysics
dc.titleVLBI observations of nineteen GHz-Peaked-Spectrum radio sources at 1.6 GHz
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