CO Modelling of CW Leo
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.
- Publication:
-
Astrophysics and Space Science
- Pub Date:
- February 1995
- DOI:
- 10.1007/BF00667910
- Bibcode:
- 1995Ap&SS.224..471G
- Keywords:
-
- CO observations;
- stars: AGB;
- stars: individual: CW Leo;
- mass loss