No CrossRef data available.
Article contents
The Influence of Dust Properties on the Mass Loss in Pulsating AGB Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
We are currently studying carbon based dust types of relevance for carbon-rich AGB stars, to obtain a better understanding of the influence of the optical and chemical properties of the grains on the mass loss of the star. An investigation of the complex interplay between hydrodynamics, radiative transfer and chemistry has to be based on a better knowledge of the micro-physics of the relevant dust species.
- Type
- Part 5. Mass Loss in Pulsating Stars
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2002
References
You have
Access