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The Carbon Stars Adventure
Modelling C-star atmospheres†
Published online by Cambridge University Press: 27 October 2016
Abstract
We compare in a systematic way spectrometric, photometric and mid-infrared (VLTI/MIDI) interferometric measurements with different types of model atmospheres. Self-consistent dynamic model atmospheres in particular were used to interpret in a consistent way the dynamic behavior of gas and dust. The results underline how the joint use of different kind of observations, as photometry, spectroscopy and interferometry, is essential to understand the atmospheres of pulsating C-rich AGB stars. The sample of C-rich stars discussed in this work provides crucial constraints for the atmospheric structure.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 160 - 161
- Copyright
- Copyright © International Astronomical Union 2016
Footnotes
This work is supported by the Austrian Science Fund FWF under project number P23006-N16.