The GALEX/FUV maps of Centaurus A. Left: The overall map of Centaurus A. Yellow squares correspond to the northeast and the southwest region investigated in this paper, as in Fig. 2, for both of which past studies suggest that jet-induced star formation may have occurred therein. Right: Enlarged FUV maps of the northeast (top), the southwest (center), and the central (bottom) region. The yellow contours show the Herschel 250 μm intensity distribution, the levels of which correspond to 9, 10.5, 12, and 18 MJy sr⁻¹. The black ellipse in the bottom panel is the photometry aperture to measure the FUV flux from the central region of Cen A. All the FUV images in the left and right panels are shown after smoothed with a Gaussian kernel of $4\stackrel{″}{.}5$.