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Fig. 5

image

Surface brightness radial profiles of NGC 4371, derived from ellipse fits to the HST image. The right panels focus on the inner 30′′ (shaded area on the left panels). Bottom panels have the radial axis displayed on a log scale. The vertical dashed lines indicate the positions of the nuclear features seen in the position angle and ellipticity radial profiles derived from the HST image (see Fig. 6).

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