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CO modelling of CW leo
Authors:Martin Groenewegen
Institution:(1) Institut d'Astrophysique de Paris, 98 bis Boulevard Arago, F-75014 Paris, France
Abstract:Preliminary results are presented of fitting the spectral energy distribution and newly obtained12CO and13CO J =1-0, 2-1 and 3-2 line profiles of CW Leo. This is done with a model which includes a self-consistent calculation of the gas temperature.
Keywords:CO observations  stars: AGB  stars: individual: CW Leo  mass loss
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