Image Details
Caption: Figure 5.
Contours of the integrated CO(1–0) flux in NGC 2865 superposed on an HST WFPC F555W image. The dust lane lies along PA −30°, with the more obscured near side of the disk being offset by 0﹩\mathop{.}\limits^{{\unicode{x02033}}}﹩2 (in projection) from the galaxy nucleus.
© 2026. The Author(s). Published by the American Astronomical Society.