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The JCMT Gould Belt Survey: Evidence for radiative heating and contamination in the W40 complex

D. Rumble,J. Hatchell,K. Pattle,Helen Kirk,Tom J. Wilson,J. V. Buckle,David Berry,H. Broekhoven-Fiene,M. J. Currie,M. Fich,T. Jenness,D. Johnstone,J. C. Mottram,D. Nutter,Jaime E. Pineda,C. Quinn,C. Salji,S. Tisi,S. Walker-Smith,J. Di Francesco,M. R. Hogerheijde,Derek Ward-Thompson,Pierre Bastien,D. Bresnahan,Harold M. Butner,M. Chen,A. Chrysostomou,S. Coude,Christopher J. Davis,Emily Drabek-Maunder,A. Duarte-Cabral,Jason D. Fiege,Per Friberg,R. Friesen,G. A. Fuller,S. Graves,J. S. Greaves,J. Gregson,Wayne S. Holland,G. Joncas,Jason Matthew Kirk,Lewis B. G. Knee,S. Mairs,Kenneth A. Marsh,Brenda C. Matthews,G. Moriarty-Schieven,C. Mowat,J. M. C. Rawlings,J. S. Richer,D. Robertson,Erik Rosolowsky,S. Sadavoy,H. Thomas,N. F. H. Tothill,S. Viti,G. J. White,J. Wouterloot,J. A. Yates,M. Zhu

Monthly Notices of the Royal Astronomical Society（2016）

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Abstract
We present SCUBA-2 450 μm and 850 μm observations of the W40 complex in the Serpens-Aquila region as part of the James Clerk Maxwell Telescope (JCMT) Gould Belt Survey (GBS) of nearby star-forming regions. We investigate radiative heating by constructing temperature maps from the ratio of SCUBA-2 fluxes using a fixed dust opacity spectral index, β = 1.8, and a beam convolution kernel to achieve a ...
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Key words
radiative transfer,catalogues,stars: formation,H ii regions,submillimetre: general
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