Image Details
Caption: Fig. 8.
12.5 μm emission from G45.12 (gray scale, smoothed to 2﹩\arcsec﹩) vs. 1.3 cm radio continuum emission (contours, ~2﹩\farcs﹩5 beam; adapted from Fig. 1 of Hofner et al. 1999). The small white pluses are the mid‐IR sources discussed in the text; the large black pluses are the outflow centers found by Hunter, Peterson, & Cesaroni (1997).
© 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.