The galaxy pair associated with NGC 7268 (see Fig. 10) has a foreground
SB ringed galaxy with a recession velocity 400 km s^-1^ greater than
that of the background S0/E galaxy. Results were obtained for two
regions, each 1.56" (~1 kpc) wide and not sharing any pixels. The
location of these areas with respect to galaxy features appears to be in
the outer ring of the foreground barred galaxy. The average ring
extinctions are A_B_ = 0.53 (using the intensity profile method) and
A_B_ = 0.30 (using the B-image/spectrum method). The face-on-corrected
values are A_B_ = 0.35 and A_B_ = 0.21, given an axial ratio of
a/b = 1.50.
Double system, interacting(?) pair at 0.4 with small bright companion.
Note 1m correction to NGC RA.
Interacting pair at 0.35. In cluster. 1 min error in NGC RA.
=ESO 467-IG 57
*NGC RA 1.0 minutes off