Saraceno, P.; Nisini, B.; Benedettini, M.; di Giorgio, A. M.; Giannini, T.; Kaufman, M. J.; Lorenzetti, D.; Molinari, S.; Pezzuto, S.; Spinoglio, L.; Tommasi, E.; Caux, E.; Ceccarelli, C.; Clegg, P. E.; Correia, J. C.; Griffin, M. J.; Leeks, S. J.; Liseau, R.; Smith, H. A. and White, G. J.
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We review the results of the observations in the 45-190 μm wavelength range with the ISO Long Wavelength Spectrometer of a sample of Class 0, Class I, Class II pre-Main Sequence objects. We briefly discuss the role of [OI] and of molecular lines in the cooling of these sources.
|Item Type:||Conference Item|
|Copyright Holders:||1999 European Space Agency|
|Extra Information:||Proceedings of the Conference "The Universe as seen by ISO", Paris, France, 20-23 October 1998
ESA SP-427, March 1999
|Keywords:||stars; circumstellar matter; pre-main sequence; infrared; spectroscopy; molecular lines|
|Academic Unit/School:||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:||03 May 2012 14:51|
|Last Modified:||29 Nov 2016 22:03|
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