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Dust Formation in WC-Star Shells

Published online by Cambridge University Press:  03 August 2017

E. Sedlmayr  and
H. Gass
E. Sedlmayr
Affiliation:
Institut für Astronomie und Astrophysik Technische Universität Berlin, PN 8-1 Hardenbergstraße 36 D-1000 Berlin 12
H. Gass
Affiliation:
Institut für Astronomie und Astrophysik Technische Universität Berlin, PN 8-1 Hardenbergstraße 36 D-1000 Berlin 12

Abstract

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The conditions of dust formation in the winds of WC-stars are discussed. Simple analytical estimations for the existence of neutral carbon zones where carbon nucleation might occur are given. It is shown that efficient dust formation can take place in the CI region if the effective temperature of the star is below ~ 25000 K and the density at the base of the wind is larger than ~ 1011 cm–3.

Type
Session VI. Enrichment
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 335 - 340
Copyright
Copyright © Kluwer 1991 

References

Bode, M.F., Evans, A.: 1983, Quart. J. Roy. astr. Soc. 24, 83 Google Scholar
Chiosi, C., Maeder, A.: 1986, Ann. Rev. Astron. Astrophys. 24, 329 CrossRefGoogle Scholar
Gail, H.-P., Sedlmayr, E.: 1988, Astron. Astrophys. 206, 153 Google Scholar
Maeder, A., Meynet, G.: 1987, Astron. Astrophys. 182, 243 Google Scholar
Williams, P.M., van der Hucht, K.A., The, P.S.: 1987, Astron. Astrophys. 182, 91 Google Scholar