Image Details
Caption: Fig. 3.
Mid‐IR emission from G45.07. Three compact mid‐IR components are detected at both 12.5 (upper left; ﹩0.6< F< 39﹩ mJy pixel−1) and 20.6 μm (upper right; ﹩4.4< F< 158﹩ mJy pixel−1). Color temperature (lower left; ﹩105< T_{d}< 165﹩ K, contours at 100, 110, 120, 130, 140, and 150 K), and opacity (lower right; ﹩1.4< \tau _{12.5}< 160\times 10^{-3}﹩, contours at 0.5, 1.0, 2.0, 4.0, and ﹩10.0\times 10^{-3}﹩) maps are also shown. To better show the extended emission, G45.07 KJK 1 and 2 are saturated in the 12.5 μm image and KJK 1 in the 20.6 μm image. (The ringlike structure centered on KJK 1 in the temperature map is an artifact due to the beam‐matching process.) In Figs. 4–7, darker is brighter, hotter, or more opaque, as appropriate; flux and opacity gray scales are logarithmic; cores may be saturated to show the extended emission; and compact mid‐IR sources are indicated with pluses and labeled in the opacity maps.
© 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.