Structure and kinematics of edge-on galaxy discs – I. Observations of the stellar kinematics

• Published in: Monthly notices of the Royal Astronomical Society 2004-07, Vol.351 (4), p.1247-1265
• Main Authors: Kregel, M., Van Der Kruit, P. C., Freeman, K. C.
• Format: Article
• Language: English
• Subjects: galaxies: fundamental parameters; galaxies: kinematics and dynamics; galaxies: spiral; galaxies: structure
• ISSN: 0035-8711; 1365-2966
• DOI: 10.1111/j.1365-2966.2004.07864.x

We present deep optical long-slit spectra of 17 edge-on spiral galaxies of intermediate to late morphological type, mostly parallel to their major axes and in a few cases parallel to the minor axes. The line-of-sight stellar kinematics are obtained from the stellar absorption lines using the improved cross-correlation technique. In general, the stellar kinematics are regular and can be traced well into the disc-dominated region. The mean stellar velocity curves are far from solid-body, indicating that the effect of dust extinction is not large. The line-of-sight stellar disc velocity dispersion correlates with the galaxy maximum rotational velocity, but detailed modelling is necessary to establish whether this represents a physical relation. In four spirals with a boxy- or peanut-shaped bulge we are able to detect asymmetric velocity distributions, having a common signature with projected radius in the mean line-of-sight velocity and the h3 and h4 curves. In two cases this kinematic asymmetry probably represents the ‘figure-of-eight’ pattern synonymous with a barred potential. We emphasize, however, that the signatures seen in the h3 and h4 curves may also be due to the disc seen in projection.