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Synthetic AGB Evolution in the LMC: The Abundances of PN

Published online by Cambridge University Press:  07 August 2017

Martin Groenewegen  and
Teije De Jong
Martin Groenewegen
Affiliation:
Astronomical Institute, Kruislaan 403, NL-1098 SJ Amsterdam, Holland
Teije De Jong
Affiliation:
Astronomical Institute, Kruislaan 403, NL-1098 SJ Amsterdam, Holland SRON, Space Research Groningen, P.O. Box 800, NL-9700 AV Groningen, Holland

Extract

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We have developed a model to calculate the evolution of AGB stars in a synthetic way. The evolution is started at the first thermal pulse (TP) and ends when the envelope mass has been lost due to mass loss or when the core mass reaches the Chandrasekhar mass.

Type
VI. Planetary Nebulae in Galactic Systems
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 585
Copyright
Copyright © Kluwer 1993