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Theoretical models of the Planetary Nebula populations in galaxies

Published online by Cambridge University Press:  25 May 2016

M. G. Richer ,
M. L. McCall  and
N. Arimoto
M. G. Richer
Affiliation:
1Observatoire de Meudon
M. L. McCall
Affiliation:
2York University
N. Arimoto
Affiliation:
3University of Tokyo

Extract

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We consider the possibility of using bright planetary nebulae to study the chemical evolution of their parent galaxies. In particular, we would like to use planetary nebulae as abundance probes in galaxies where star formation ended long ago, such as ellipticals or the bulges of spirals, and in which no other direct probes exist. However, if we are to use planetary nebulae to study the chemical evolution of their parent galaxies, we must relate the oxygen abundance in bright planetary nebulae to the oxygen abundance in the interstellar medium when star formation stopped. Obviously, only theoretical modelling can provide this information once star formation has stopped.

Type
VIII. Planetary Nebulae in Extragalactic Systems
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 474
Copyright
Copyright © Kluwer 1997 

References

Arimoto, N., Yoshii, Y., & Takahara, F. 1992, A&A, 253, 34.Google Scholar
Richer, M. G., McCall, M. L., & Arimoto, N. 1996, A&AS, in press.Google Scholar