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EnglishWe 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 UGC 10205 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.
| Titolo: | Figure-of-eight velocity curves: UGC 10205 | |
| Autori: | ||
| Data di pubblicazione: | 1997 | |
| Rivista: | ||
| 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 UGC 10205 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. | |
| Handle: | http://hdl.handle.net/11577/2458983 | |
| Appare nelle tipologie: | 01.01 - Articolo in rivista |
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