Image Details
Caption: Fig. 5.
Plot of ﹩K_{s}﹩ vs. ﹩K_{s}-[ 24] ﹩ for all of the objects considered here. Plus signs are objects from the BPMG; circles are objects from Tuc‐Hor. The objects with excesses at 24 μm, selected by a combination of techniques, are indicated by name; see text for discussion as to how the objects with excesses were selected.
© 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.