Kinematic Analysis of the Double-Barred Galaxy NGC 357

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We present a kinematic analysis of the double-barred early-type galaxy NGC 357. The radial velocity and velocity dispersion profiles along both the nuclear bar axis and the semi-major axis clearly reveal the presence of the two bars. The results indicate that the bulge is pressure supported whereas the |vr|/σ ratio shows a plateau along the nuclear bar.

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