A catalog of dusty elliptical galaxies is presented in
[32] where
the authors also classify the objects based on the relative
disposition and morphology of the dust distribution as given in the table
below.
Click here for the
NED
listing of the Dusty Ellipticals cited in
Ebneter, K., & Balick, B. 1985, Astron. J., 90, 183.
A selection of additional papers discussing Dust-Lane Ellipticals include:
Dusty Ellipticals
Type Definition
O Oblate - dust lane lies parallel to the optical major
axis of the galaxy (this class may be contaminated by normal S0 or Sa
galaxies.)
P Prolate - dust lane lies parallel to the optical minor
axis of the galaxy.
S Skew - dust lane does not lie parallel to either optical
axis of the galaxy.
I Indeterminate - stellar component of galaxy appears
spherical; dust is in a well-defined lane.
D Diffuse - dust is distributed in irregular patches in
the galaxy.
M Multiple - galaxy has two dust lanes: one on the optical
major axis, one on the optical minor axis.
W Warped - dust lane is warped.
BE Bright Edge - dust lane has a bright edge, possibly due
to a stellar disk.
U Unknown - dust type could not be determined, but galaxy
has been identified as containing dust.
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