The counter-rotating stellar core of NGC 4494 | Astronomy & Astrophysics (A&A)

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Fig. 4.

As in Fig. 2, but for a counter-rotating stellar component. The radial profile of f₁₂ in the middle panel indicates that the contribution of the counter-rotating component is null within the central $| R | < 1 \overset{″}{.} 5$ $|R| < 1{{\overset{\prime\prime}{.}}}5$ and then rises and matches the flux of the host galaxy at |R|≃6″. Outwards, it declines until disappearing for |R|> 18″.

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