Letter to the Editor
ISO-SWS *spectra of the C-rich AGB star R Scl and dynamical model atmospheres
J. Hron 1,
R. Loidl 1,
S. Höfner 2, 1,
U.G. Jorgensen 2,
B. Aringer 1 and
F. Kerschbaum 1
Received 12 May 1998 / Accepted 22 May 1998
We have monitored the spectral variations of the carbon rich AGB star R Scl in the 2-45 µm range using the ISO-SWS instrument. We have also computed hydrostatic and hydrodynamic model atmospheres and corresponding synthetic spectra representative for two phases of R Scl. There is good qualitative agreement between observations and models in the near IR. This demonstrates the theoretical progress and the potential of analysing carbon star spectra with self-consistent dynamical models.
Key words: stars: AGB and post-AGB stars: atmospheres hydrodynamics molecular processes stars: variables infrared: stars
* Based on observations with ISO, an ESA project with instruments funded by ESA member states (especially the PI countries: France, Germany, the Netherlands and the United Kingdom) and with the participation of ISAS and NASA.
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© European Southern Observatory (ESO) 1998
Online publication: June 26, 1998