Fig. B.1.

Stellar kinematics and line-strength indices measured along the major (top panels), diagonal (middle panels) and minor axis (bottom panels) of NGC 6482. For each axis, the curves are folded around the nucleus. Blue asterisks and red circles refer to data measured along the approaching and residing sides of the galaxy, respectively. The left panels (from top to bottom) show the radial profiles of the mean velocity (ν) after the subtraction of the systemic velocity, velocity dispersion (σ), third- and fourth-order coefficients of the Gauss–Hermite decomposition of the LOSVD (h3 and h4). The right panels (from top to bottom) show the radial profiles of the line-strength indices Hβ, [MgFe]′, 〈Fe〉, Mgb, and Mg2. The vertical dotted line corresponds to the effective radius re of the spheroidal component. The name of the galaxy and orientation of the slit are given for each data set.
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