Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-11-20
Astronomy and Astrophysics
Astrophysics
8 pages, 7 figures to be published in Astronomy & Astrophysics
Scientific paper
The 13-16 um region observed by the Infrared Space Observatory (ISO) of several ABG stars are discussed. We present and analyse spectra of seven M giants which show carbon dioxide features. To explain the features of the bands, we suggest they originate from two different circumstellar layers, one being a warm and high density layer close to the star, possibly making the 15 um band optically thick, and the other being a large, cold and optically thin layer extending far out in the wind. This could explain the difference in temperatures of the different bands found in the analysis of the spectra and the number of molecules needed for the emission. It is demonstrated that in spite of the bands probably not being formed in vibrational LTE, the temperatures can be estimated from the widths of the bands.
Eriksson Kimmo
Gustafsson Bengt
Ryde Nils
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