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Formation and Evolution of Planetary Nebulae: A Radiation Hydrodynamics Study

Published online by Cambridge University Press:  26 May 2016

M. Perinotto ,
C. Calonaci ,
D. Schönberner ,
M. Steffen  and
T. Blöcker
M. Perinotto
Affiliation:
Dipartimento di Astronomia, Firenze, Italy
C. Calonaci
Affiliation:
Dipartimento di Astronomia, Firenze, Italy
D. Schönberner
Affiliation:
Astrophysikalisches Institut Potsdam, Potsdam, Germany
M. Steffen
Affiliation:
Astrophysikalisches Institut Potsdam, Potsdam, Germany
T. Blöcker
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, Germany

Abstract

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The formation and evolution of a planetary nebula is based on the occurrence of a strong AGB wind and the rapid evolution of the central star with corresponding changes of its ionizing flux and wind power. We have studied the influence of different mass-loss histories in combination with various central-star properties.

Type
Part III: Planetary Nebulae in the Scheme of Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003 , pp. 157 - 158
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

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Perinotto, M., Kifonidis, K., Schönberner, D., Marten, H. 1998, A&A 332, 1044 Google Scholar