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- W2093155291 abstract "Highly excited molecular hydrogen is observed in dense molecular clouds in star-forming regions in our own and other galaxies. It is generated in shocks caused by powerful outflows from young or prestellar objects impacting the parent cloud, and also by fluorescence from recently formed massive stars irradiating their surroundings, and creating a photodissociation region." @default.
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- W2093155291 title "Observations of molecular hydrogen in star-forming regions" @default.
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