We present high-spatial-resolution, mid-IR images of young stellar obj
ects (YSO). Images were obtained with MIRAC (Mid-InfraRed Array Camera
) at wavelengths of grain continuum and feature emission near 10 and 2
0 mu m. Three of the objects observed (WL 16, TY CrA and MWC 1080) sho
w structure and extended emission (on the order of 1200 AU or greater)
at wavelengths of the UIR (Unidentified InfraRed) emission features.
Mid-IR imaging of other sources in these clouds which do not exhibit U
IR features (ELias 29 and R CrA) shows these sources to be point-libe.
We have produced morphological models based on the mid-IR images for
the observed extended structures.