Fridlund, C. V. M. and White, G. J.
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CO and 13CO observations of the molecular outflow source L1551 IRS5 are reported. Lower limits to the mass and energetics are calculated, and these are found to be too high for the outflow to be radiatively driven by the central object. However, the values are found to be in quantitative agreement with recent far infrared results reported in the literature.
|Item Type:||Book Chapter|
|Copyright Holders:||1989 Springer|
|Extra Information:||Proceedings of a Symposium held at Zermatt, Switzerland, 22–25 September 1988 to Commemorate the 600th Anniversary of the University of Cologne and the 20th Anniversary of the Gornergrat Observatory|
|Academic Unit/Department:||Science > Physical Sciences|
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||G. J. White|
|Date Deposited:||15 Feb 2012 15:40|
|Last Modified:||23 Oct 2014 09:34|
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