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.
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. |
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: