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Abundances and gradients in nearby galaxies

Published online by Cambridge University Press:  08 August 2017

Fabio Bresolin
Fabio Bresolin*
Affiliation:
Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, 96822 Honolulu, HI, USA email: bresolin@ifa.hawaii.edu
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Abstract

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The study of chemical abundance gradients can provide essential information on the evolution of disk galaxies. Here I briefly review our current observational knowledge concerning the abundances of the ionized gas (H ii regions and planetary nebulae) in nearby galaxies, and how they inform us about the time evolution of metallicity gradients.

Keywords

galaxies: spiralgalaxies: evolutionISM: abundances
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. 237 - 244
Copyright
Copyright © International Astronomical Union 2017 

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