We measured detailed velocity and velocity dispersion curves and line-profile shapes of the ionized gas in the central region of the edge-on Sa galaxy UGC 10205. These observations allow to establish that in this early-type spiral three distinct kinematic gaseous components are present.
Evidence for distinct kinematic gaseous components in disk galaxies
CORSINI, ENRICO MARIA;PIZZELLA, ALESSANDRO;BERTOLA, FRANCESCO
1997
Abstract
We measured detailed velocity and velocity dispersion curves and line-profile shapes of the ionized gas in the central region of the edge-on Sa galaxy UGC 10205. These observations allow to establish that in this early-type spiral three distinct kinematic gaseous components are present.
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1997_ASPC_117_167_VegaBeltran_U10205.pdf
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