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2017MNRAS.465.2277P - Mon. Not. R. Astron. Soc., 465, 2277-2285 (2017/February-3)
Using CO line ratios to trace the physical properties of molecular clouds.
PENALOZA C.H., CLARK P.C., GLOVER S.C.O., SHETTY R. and KLESSEN R.S.
Abstract (from CDS):
Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): molecular processes - stars: formation - ISM: clouds - ISM: evolution - ISM: evolution
Simbad objects: 4
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