White, Glenn J.; Phillips, J. P.; Richardson, K. J. and Harten, R. H.
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A survey of the CO J= 4-3 transition has been made towards a sample of seven galactic molecular clouds. These data have been combined with spectra for the lower CO transitions to examine how they vary in line shape with different transition. Such variations are examined using LVG modelling techniques to obtain estimates of the physical state of the emitting gas. The authors discuss the implications and importance that observations of these submillimetre wavelength transitions have in refining knowledge of the gas in molecular clouds.
|Item Type:||Journal Article|
|Copyright Holders:||1986 European Southern Observatory|
|Keywords:||astronomical spectroscopy; carbon monoxide; interstellar gas; molecular clouds; line spectra; Ophiuchi clouds; spectral line width|
|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:||04 May 2012 09:21|
|Last Modified:||29 Nov 2016 04:51|
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