4.2 Other Galaxies
As discussed already above, for NGC 4414 I find a mean Q of about
1.15 for a ``maximum disc'' model, and about 2.30 for a ``no m = 2''
model. For NGC 2841, a preliminary analysis shows that for a ``maximum
disc'' model Q 1.5-1.6, so
that here a ``no m = 2'' model is
dynamically too hot to be acceptable. Further work on other galaxies
is in progress. In all cases, spectra are taken along the minor
and the major axes, since only their combination can help us
disentangle the radial, azimuthal and perpendicular velocity dispersions
(cf. work on NGC 488 by
Gerssen et al. 1997).
It is hoped that
with such data, a clearer answer can be given to the question
whether the disc is close to ``maximum disc'' or not.