NGC 2264 G
NGC 2264 G: (a) The 4.5 μm and 24 μm HiRes deconvolved images. There is no MIPS data for this source. Only the IRAC 4.5 μm gray scale image is shown. A square root color stretch is used to bring out low and high brightness emissions and the contour levels are in increments of factors of two or larger as indicated. The peak intensities (in units of MJy Sr–1) in the protostar/jet-outflow are indicated. (b) 3-color representation of HiRes deconvolved Spitzer IRAC images: IRAC 3.6 μm (blue), 4.5 μm (green), 8.0 μm (red). In the 3-color representation the wide angle outflows are identified by the blue excess while the h2 jets and bow shocks by the green excess.
