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The chemistry of dust formation in red supergiants

Published online by Cambridge University Press:  23 May 2013

I. Cherchneff
I. Cherchneff*
Affiliation:
Physik Departement, Universität Basel, Klingelbergstrasse 82, 4056 Basel, Switzerland
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Abstract

Massive stars in their late stages of evolution as Red Supergiants experience mass loss. The resulting winds show various degrees of dynamical and chemical complexity and produce molecules and dust grains. This review summarises our knowledge of the molecular and dust components of the wind of Red Supergiants, including VY CMa and Betelgeuse. We discuss the synthesis of dust as a non equilibrium process in stellar winds, and present the current knowledge of the chemistry involved in the formation of oxygen-rich dust such as silicates and metal oxides.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 60: Betelgeuse Workshop 2012 The Physics of Red Supergiants: Recent Advances and Open Questions , 2013 , pp. 175 - 184
Copyright
© EAS, EDP Sciences 2013

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