Free Access
Volume 532, August 2011
Article Number A38
Number of page(s) 31
Section Extragalactic astronomy
Published online 19 July 2011

Online material

thumbnail Fig. 1

Naturally weighted CLEAN images of the observed sources between 1.4 and 15 GHz. The lowest contour value “clev” is chosen at four times the rms noise, the peak brightness is given by “max”. The contour levels increase by factors of two. The dashed contours indicate negative brightness. The beam’s full width at half maximum (FWHM) is shown in the bottom left corner of the images in gray. An epoch of observation is shown in the bottom right corner. Red and blue spots indicate the positions and sizes (FWHM) of Gaussian model components for the core and the jet features, respectively.

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© ESO, 2011

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