Fridlund, C. V. M. and White, G. J.
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New high-signal/noise 13CO observations of the bipolar outflow in the molecular cloud L1551 are reported. Contrary to earlier observations of CO J = 1-0 and 2-1, no strong spatial dependence is found for the velocity profile of these spectra. The implications of these observations are such that the model of an empty shell for this source is less likely, and a model consisting of a shell which contains significant amounts of outflowing molecular gas inside the swept-up cavity walls is suggested.
|Item Type:||Journal Article|
|Copyright Holders:||1989 European Southern Observatory|
|Keywords:||carbon monoxide; interstellar gas; molecular clouds; signal to noise ratios; Herbig-Haro objects; molecular spectra; optical thickness; spatial distribution; velocity distribution|
|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:||18 May 2012 09:54|
|Last Modified:||05 Oct 2016 01:18|
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