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- W2040304709 abstract "We have scanned the region around the OH maser source DR21 (OH) with a 20-arcsec beam at a wavelength of 350μm and discovered a hitherto unknown double structure, with two peaks of roughly equal mass separated by 40 arcsec (0.1 pc) in declination. The northernmost peak is coincident with the OH maser position and the centroid of the far-infrared emission, while the southern source has not previously been found at any wavelength. Both sources are extremely dense and deeply embedded, with optical depths of order unity even in the far-infrared. The southern source may be one of the densest molecular cores yet found, and is a candidate protostar. These results confirm that OB star formation can occur deep within molecular clouds, and not just at their edges." @default.
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- W2040304709 date "1988-03-01" @default.
- W2040304709 modified "2023-10-01" @default.
- W2040304709 title "Submillimetre observations reveal that DR21 (OH) is a double source" @default.
- W2040304709 doi "https://doi.org/10.1093/mnras/231.1.47p" @default.
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