Figure-of-eight velocity curves: UGC10205

J. C. Vega; E. M. Corsini; A. Pizzella; F. Bertola

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arXiv · astro-ph/9705047

Figure-of-eight velocity curves: UGC10205

J. C. Vega·E. M. Corsini·A. Pizzella·F. Bertola

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Abstract

We measured the velocity curve and the velocity dispersion profile of the ionized gas along the major axis of the edge-on galaxy UGC~10205. The observed kinematics extends up to about 40 arcsec from the nucleus. In the inner 13 arcsec of this early-type spiral three kinematically distinct gaseous components are present. We disentangle a fast-rotating and a slow-rotating component. They give to the UGC10205 velocity curve a ``figure-of-eight'' appearance. A third velocity component is also detected on the southeast side of the galaxy. Possibly it is produced by gas in non-circular motions.

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J. C. Vega, E. M. Corsini, A. Pizzella, F. Bertola. 1997-05-07. Figure-of-eight velocity curves: UGC10205. https://arxiv.org/abs/astro-ph/9705047

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