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Astron. Astrophys. 337, 149-177 (1998)

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Acknowledgements

We are indebted to H. Yorke for the permission to modify his original code and to apply it to the problem of dusty stellar outflows. We thank T. Blöcker for providing us with the data from his stellar evolution calculations with mass loss. Part of this research is funded by "Deutsche Agentur für Raumfahrtangelegenheiten (DARA) under grant 50 OR 9411. One of us (R. Sz.) expresses his gratitude to the Canadian Institute of Theoretical Astrophysics, to the Astrophysical Institute Potsdam, and to the Polish State Committee for Scientific Research - grants No. 2.P03D.027.10 and 2.P03D.002.13. M.S. gratefully acknowledges the the hospitality and support provided by the Nicolaus Copernicus Astronomical Center, Torun.

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© European Southern Observatory (ESO) 1998

Online publication: August 6, 1998
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