Fig. 7
Left panel: HST B-band image of S443 (at the
top) and S442 (bottom). Black contours (starting at
0.1 mJy and increasing by factors of 
) represent the ATCA 1.4 GHz flux
density and the cross indicates the S443 VLBI position. Right
panel: an enlarged region of the HST image of S443 with enhanced
contrast and a cross indicating the VLBI position, which is at the very edge of
the galaxy, but not outside it.
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