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Fig. 6.

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Position angle as a function of distance along the major axis for the ellipse fit of the HST imaging of NGC 1277 (left) and NGC 1278 (right). The error bars correspond to the one-sigma uncertainties. The vertical dashed lines indicate the radial interval over which the kinematical axis was determined. Its estimated value is indicated by the number in the lower part of the panels and the horizontal dotted lines.

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