… KG Begeman Kapteyn Astronomical Institute, Groningen University, Postbus 800, NL-9700
AV Groningen, The … value for 8max for galaxies with moderate warps used in this thesis …

… In fitting dark-halo models we follow essentially the procedure outlined by Begeman (1987).
We assume that the halo is spherical and has a density distribution given by a form which is …

We propose a form for dark haloes that embodies the fundamental aspect of Milgrom's
modified dynamics (MOND): the discrepancy between the visible mass and the Newtonian …

… in many luminous nearby disc galaxies (eg Begeman 1987; Broeils 1992). The projected …
dominates the surface mass density (eg Begeman 1987; Broeils 1992). The oblateness q …

Asymmetries in the distributions of light and neutral hydrogen are often observed in disk
galaxies. But how common are they? It is possible to estimate their number? Lopsided HI …

… In order to determine the kinematical parameters and the rotation curve of NGC 2403, we
have performed the standard tiltedring fit of the velocity field (Begeman 1987). The rings have …

… existing literature (Begeman there is sufficient spatial resolution; the HI distribu- 1987): tion
… rotation curves, the advice and help of KG Begeman is invaluable. I thank him especially for …

… Begeman 1987). One can also keep the geometry for the whole disk fixed, and fit a single
shape to the rotation curve (see eg van Moorsel & Wells 1985). This will generally result in a …

… We have included NGC 5371 (Begeman 1987), which was not used by Broeils ‘because
of its clumpy gas distribution and asymmetric velocity field’. For our purpose the properties of …

… here under the terms of Article 25fa of the Dutch Copyright Act, indicated by the “Taverne”
license. More information can be found on the University of Groningen website: https://www.rug…