Fig. 1
Three-colour image of the Corona Australis molecular cloud. In purple/blue and is Spitzer 24-μm emission. Orange and yellow emission denotes SPIRE 160-μm emission. Red indicates SPIRE 250-μm emission. The northern tail, southern streamer, and westernmost filament or streamer are labelled. A bar indicating the length of 1 pc has been included to the lower left, and the relative orientation of the galactic coordinate system is shown to the lower right.
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