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Cited article:

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SEARCHING FOR THE DRIVING SOURCE OF THE CO MOLECULAR OUTFLOW IN THE HIGH-MASS STAR-FORMING REGION G240.31+0.07

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SUBMILLIMETER ARRAY OBSERVATIONS OF THE MOLECULAR OUTFLOW IN HIGH-MASS STAR-FORMING REGION G240.31+0.07

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Outflow and Infall in a Sample of Massive Star‐forming Regions

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654 GHz Continuum and C 18 O(6-5) Observations of G240.31+0.07 with the Submillimeter Array

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Submillimeter Array Outflow/Disk Studies in the Massive Star-forming Region IRAS 18089-1732

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