Abstract
Maps in the mid-infrared and submillimetre thermal continuum are presented for the star-forming region W75N. Observations at 10 and 20 μm, with ∼ 5-arcsec resolution, trace warm dust heated by members of the embedded young stellar cluster. The submillimetre continuum emission traces the cool dust in the cloud core surrounding the luminosity sources. The core has been spatially resolved at 350 μm but shows no disc-like structure related to the known molecular outflow on scales larger than ∼ 0.2 pc.
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