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Planetary Nebulae as Tracers of Chemical Evolution in External Galaxies

Published online by Cambridge University Press:  26 May 2016

Marshall L. McCall  and
Michael G. Richer
Marshall L. McCall
Affiliation:
York University, Department of Physics and Astronomy, 4700 Keele Street, Toronto, Ontario, Canada M3J 1P3 mccall@yorku.ca
Michael G. Richer
Affiliation:
Observatorio Astronómico Nacional, Instituto de Astronomía, UNAM, P.O. Box 439027, San Diego, CA, U.S.A. 92143-9027 richer@astroscu.unam.mx

Abstract

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Thanks to recent advances in instrumentation, metal abundances now can be measured routinely for PNe situated in galaxies beyond the Magellanic Clouds. Consequently, PNe are becoming a valuable tool for studying the chemical evolution of external galaxies, especially those which are not forming stars. Here we review problems and progress in this exciting nascent field of interdisciplinary research.

Type
Part VIII: Planetary Nebulae as Galaxy Probes
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003 , pp. 583 - 592
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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