1997
Formation of dust particles in cool stellar outflows
E. Sedlmayr and D. Krüger
in Astrophysical Implications of the Laboratory Study of Presolar Materials. St. Louis, MO, October 1996. Edited by Thomas J. Bernatowicz and Ernst Zinner. Woodbury, N.Y. : American Institute of Physics, c1997., p.425
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Abstract:
Radiative Heating and Cooling in Circumstellar Envelopes
Peter Woitke
Dissertation, Technische Universität Berlin, 1997
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Abstract:
This thesis investigates the thermal state of diluted gases being exposed to stellar radiation fields. On the basis of a steady-state non-LTE description, the radiative heating and cooling rates of the gas are determined, considering the typical densities present in circumstellar envelopes.
Radiative Heating and Cooling in Circumstellar Envelopes
Peter Woitke
Dissertation, Technische Universität Berlin, 1997
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Zusammenfassung:
Formation of small iron clusters in circumstellar envelopes.
M. John and E. Sedlmayr
Proceedings contribution to the UMIST workshop Dust and molecules in evolved stars in Manchester, 27.-29. March 1997.
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Cool star winds and mass loss: Theory
E. Sedlmayr and J.M. Winters
IX-th. EADN Summer School on "Stellar atmospheres: Theory and observations", Lecture Notes in Physics, De Greve, J.P., Blomme, R., Hensberge, H. (Eds.), Springer, 1997, p89-131
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Circumstellar dust shells around long-period variables: V. A consistent time-dependent model for the extreme carbon star AFGL 3068
J.M. Winters, A.J. Fleischer, T. Le Bertre and E. Sedlmayr
Astronomy & Astrophysics, 326, 305-317 (1997)
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Abstract:
MgO dust nucleation in M-Stars: Calculation of cluster properties and nucleation rates
M. Köhler, H.-P. Gail, and E. Sedlmayr
Astronomy & Astrophysics, 320, 553-567 (1997)
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Abstract:
Two-fluid models for stationary dust driven winds: II. The grain size distribution in consideration of drift
D. Krüger and E. Sedlmayr
Astronomy & Astrophysics, 321, 557-567 (1997)
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Abstract:
A multicomponent method for the description of the evolution of the grain size distribution in consideration of a size dependent grain drift and growth rate is applied in order to model dust driven winds around cool C-stars.