Figure-of-eight velocity curves: UGC10205

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dc.creatorVega, J. C.
dc.creatorCorsini, E. M.
dc.creatorPizzella, A.
dc.creatorBertola, F.
dc.date1997-05-07
dc.date.accessioned2026-07-07T02:23:20Z
dc.date.available2026-07-07T02:23:20Z
dc.descriptionWe 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.
dc.description8 pages, 3 figures, Latex macro A&A and psfig macro to insert figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9705047
dc.identifierhttp://arxiv.org/abs/astro-ph/9705047
dc.identifierVega et al. 1997, A&A, 324, 485
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11210
dc.subjectAstrophysics
dc.titleFigure-of-eight velocity curves: UGC10205
dc.typetext

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