A&A 408, 873-885 (2003)
DOI: 10.1051/0004-6361:20030951
Minor-axis velocity gradients in spirals and the case of inner
polar disks
E. M. Corsini, A. Pizzella, L. Coccato and F. Bertola Dipartimento di Astronomia, Università di Padova, vicolo dell'Osservatorio 2, 35122 Padova, Italy
(Received 4 March 2003 / Accepted 3 June 2003)
Abstract
We measured the ionized-gas and stellar kinematics along the major and
minor axis of a sample of 10 early-type spirals. Much to our surprise
we found a remarkable gas velocity gradient along the minor axis of 8
of them.
According to the kinematic features observed in their ionized-gas
velocity fields, we divide our sample galaxies in three classes of
objects. (i) NGC 4984, NGC 7213, and NGC 7377 show an overall velocity
curve along the minor axis without zero-velocity points, out to the
last measured radius, which is interpreted as due to the warped
structure of the gaseous disk. (ii) NGC 3885, NGC 4224, and NGC 4586
are characterized by a velocity gradient along both major and minor
axis, although non-zero velocities along the minor axis are confined
to the central regions. Such gas kinematics have been explained as
being due to non-circular motions induced by a triaxial
potential. (iii) NGC 2855 and NGC 7049 show a change of slope of the
velocity gradient measured along the major axis (which is shallower in
the center and steeper away from the nucleus), as well as non-zero gas
velocities in the central regions of the minor axis. This has been
attributed to the presence of a kinematically-decoupled gaseous
component in orthogonal rotation with respect to the galaxy disk,
namely an inner polar disk. The case and origin of inner polar disks
are discussed and the list of their host galaxies is presented.
Key words: galaxies: kinematics and dynamics -- galaxies: spiral -- galaxies: structure
Offprint request: E. M. Corsini, corsini@pd.astro.it
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