5.1.4 IC 1963 - Fig. 2 shows very good agreement between new measurements of
mean streaming velocity and those in D'Onofrio et al. (1995) for this rather
nondescript S0 system. The velocity dispersion measurements do not agree at all
well, but once again this conflict can be attributed to the inadequate spectral
resolution of the older data.
ESO 358-G26 and ESO 358-G29 are among the earliest galaxy types in our
sample, and do not show any evidence for a sizable amount of extinction.
The vertical colour profiles are featureless and entirely consistent
with no gradient at all (ESO 358-G26: Fig. 2e, T = -2.0;
ESO 358-G29: T = -1.6).
= IC 1963
Overexposed, slightly flattened bulge, much extended corona. Similar to
NGC 1380A and NGC 1381.
=ESO 358- G 26