Fig. 1
Composite three-color Herschel image of NGC 2264: PACS 70 and 160 μm in blue and green; SPIRE 250 μm in red. The massive star S Mon, the central protoclusters NGC 2264 IRS1 and IRS2 and the Cone Nebula are labeled. The blue component traces heated regions while earlier stage star-forming sites, such as clumps and filaments, are traced by the red component. The image has been rotated from the RA–Dec grid.
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