CO Modelling of CW Leo

Details CO Modelling of CW Leo CO Modelling of CW Leo

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..471g&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 471-472

Astronomy and Astrophysics

Astrophysics

Co Observations, Stars: Agb, Stars: Individual: Cw Leo, Mass Loss

Scientific paper

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.

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