Image Details
                    Caption: Fig. 10.
Close‐ups of TDG‐N (source 26), TDG‐S (source 33), and candidate TDGs associated with NGC 5291 showing emission at 3.6 μm (top row) and "nonstellar" emission from PAHs (bottom row). The vertical bar represents 30﹩\arcsec﹩, i.e., a linear scale of 9 kpc.
© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.