========================================================================== J/A+A/426/463 B3-VLA CSS sample (Orienti+, 2004) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table1.dat table2.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/426/463 ==========================================================================
drwxr-xr-x 17 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:57 [TAR file] -rw-r--r-- 1 cats archive 478 Dec 21 2004 .message -r--r--r-- 1 cats archive 6638 Dec 21 2004 ReadMe -rw-r--r-- 1 cats archive 270 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2348 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 1080 Jul 28 2004 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 2916 Jul 28 2004 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 15964 Jul 28 2004 tables.ps.gz [Uncompressed] -r--r--r-- 1 cats archive 6419 Jul 28 2004 tables.tex
Beginning of ReadMe : J/A+A/426/463 B3-VLA CSS sample (Orienti+, 2004) ================================================================================ The B3-VLA CSS sample. V. VLBA images at 6 and 3.6 cm. Orienti M., Dallacasa D., Fanti C., Fanti R., Tinti S., Stanghellini C. <Astron. Astrophys. 426, 463 (2004)> =2004A&A...426..463O ================================================================================ ADC_Keywords: Radio sources ; Galaxies, radio ; QSOs ; Redshifts Keywords: galaxies: active - galaxies: nuclei - radio continuum: galaxies - galaxies: quasar: general - polarization Abstract: We present the results of VLBA observations at 6 and 3.6cm for eighteen Compact Steep Spectrum radio sources (CSS) from the B3-VLA CSS sample. In most cases these VLBA images display a "Double/Triple" morphology, and the core is unambiguously detected in seven sources. Multifrequency images allow us to study the spectral properties of the individual source components and to constrain the spectral age. In lobe-dominated sources the radiative ages deduced from the synchrotron theory are in the range of up 5x10^3^ years, if equipartition magnetic field is assumed. Polarized emission is detected at a few percent level for two sources only. They were the only two sources displaying polarized emission in VLA A configuration data, and this implies that beam depolarization is not effective in reducing the integrated fractional polarization for these sources.
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