White, G. J. and Little, L. T.
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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.
|Item Type:||Journal Article|
|Copyright Holders:||1975 Gordon and Breach Science Publishters Ltd, Taylor & Francis|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||G. J. White|
|Date Deposited:||26 Mar 2012 09:35|
|Last Modified:||05 Oct 2016 05:46|
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