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Protostellar Candidates in W75N
Published online by Cambridge University Press: 04 August 2017
Extract
W75N is a highly obscured region containing far-infrared sources, masers and molecular clouds. New results are presented showing highly reddened point sources near the maser source W75N(OH). One of these sources appears to be illuminating a newly discovered reflection nebula exhibiting large scale fluorescent molecular hydrogen.
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- I. Star Forming Processes in the Solar Neighborhood
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- Copyright © Reidel 1987