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Gaseous abundances in planetary nebulae: What have we learned in the past five years?

Published online by Cambridge University Press:  08 August 2017

Gloria Delgado-Inglada
Gloria Delgado-Inglada*
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 70264, Ciudad de México, 04510, Mexico email: [email protected]
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Abstract

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Nearly 50 years ago, in the proceedings of the first IAU symposium on planetary nebulae, Lawrence H. Aller and Stanley J. Czyzak said that “the problem of determination of the chemical compositions of planetary and other gaseous nebulae constitutes one of the most exasperating problems in astrophysics”. Although the situation has greatly improved over the years, many important problems are still open and new questions have arrived to the field, which still is an active field of study. Here I will review some of the main aspects related to the determination of gaseous abundances in PNe and some relevant results derived in the last five years, since the last IAU symposium on PNe.

Keywords

ISM: abundancesplanetary nebulae: generalgalaxies: abundancesstars: AGB and post-AGBnuclear reactionsnucleosynthesisabundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S323: Planetary Nebulae: Multi-Wavelength Probes of Stellar and Galactic Evolution , October 2016 , pp. 51 - 59
Copyright
Copyright © International Astronomical Union 2017 

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