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Extragalactic planetary nebulae: Tracers of the chemical evolution of nearby galaxies

Published online by Cambridge University Press:  30 August 2012

Laura Magrini ,
Letizia Stanghellini  and
Denise R. Gonçalves
Laura Magrini
Affiliation:
INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5I-50125, Firenze, Italy email: [email protected]
Letizia Stanghellini
Affiliation:
National Optical Astronomy Observatories, Tucson, AZ 85719 email: [email protected]
Denise R. Gonçalves
Affiliation:
UFRJ - Observatório do Valongo, La. Pedro Antonio 43, 20080-090 Rio de Janeiro, Brazil Department of Physics and Astronomy, University College London, Gower Street, WC1E 6BT London, UK email: [email protected]
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Abstract

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The study of the chemical composition of Planetary Nebulae in external galaxies is of paramount importance for the fields of stellar evolution and chemical enrichment history of galaxies. In recent years a number of spectroscopic studies with 6-8m-class telescopes have been devoted to this subject improving our knowledge of, among other, the time-evolution of the radial metallicity gradient in disk galaxies, the chemical evolution of dwarf galaxies, and stellar evolution at low metallicity.

Keywords

techniques: spectroscopic; ISM: abundancesISM: evolutionHII regionsplanetary nebulae: general; galaxies: irregulargalaxies: spiralLocal Groupgalaxies: evolutiongalaxies: abundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S283: Planetary Nebulae: An Eye to the Future , July 2011 , pp. 251 - 258
Copyright
Copyright © International Astronomical Union 2012

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