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White, G. J. and Little, L. T.
(1975).
URL: http://adsabs.harvard.edu/abs/1975ApL....16..151W
Abstract
Observations of the water line emission from regions near three compact infrared sources are reported. A new water vapour source has been dicovered in S140. New components have been observed in NGC 1333, one of which decreased in intensity by a factor of 2.5 over three days. The position of the W51(N) water source differs by 9ø±10ø from that of the compact HII/infrared source IRS-2 in W51.