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Influence of the Stellar Winds on the Evolution of the Planetary Nebula Nuclei

Published online by Cambridge University Press:  07 August 2017

S.K. Górny
S.K. Górny*
Affiliation:
Nicolaus Copernicus Astronomical Center, Chopina 12/18, 87-100 Toruń, POLAND

Extract

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A grid of homogeneous models of evolution of hydrogen burning planetary nebulae nuclei, assuming different stellar winds and the zero points for the post-AGB evolution, have been constructed from original Schönberners tracks. Following a simplified line-driven wind theory the mass loss rate has been adopted to be

Type
V. Planetary Nebulae Connection: Evolution to White Dwarfs
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 483
Copyright
Copyright © Kluwer 1993