by Elvire De Beck, M. L. Boyer, V. Bujarrabal, L. Decin, J. P. Fonfría, M. Groenewegen, S. Höfner, O. Jones, T. Kamiński, M. Maercker, P. Marigo, M. Matsuura, M. Meixner, G. Quintana Lacaci Martínez, P. Scicluna, R. Szczerba, L. Velilla Prieto, W. Vlemmings, and M. Wiedner
Published onMay 31, 2019
The fundamentals of outflows from evolved stars
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Abstract
Chemical evolution of the ISM and galaxies depends critically on stellar mass loss. We describe current efforts and future needs and opportunities to characterize AGB outflows: driving mechanisms, outflow rates, underlying fundamental physical and chemical processes such as dust grain formation, and dependency of these on metallicity.
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