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Stellar yields and abundances: new directions from planetary nebulae

Published online by Cambridge University Press:  08 August 2017

Maria Lugaro ,
Amanda I. Karakas ,
Marco Pignatari  and
Carolyn L. Doherty
Maria Lugaro
Affiliation:
Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungarian Academy of Sciences, H-1121 Budapest, Hungary email: maria.lugaro@csfk.mta.hu, carolyn.doherty@csfk.mta.hu Monash Centre for Astrophysics, School of Physics and Astronomy, Monash University, VIC 3800, Australia email: amanda.karakas@monash.edu
Amanda I. Karakas
Affiliation:
Monash Centre for Astrophysics, School of Physics and Astronomy, Monash University, VIC 3800, Australia email: amanda.karakas@monash.edu Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia
Marco Pignatari
Affiliation:
E. A. Milne Centre for Astrophysics, University of Hull, Cottingham Road Hull HU6 7RXUnited Kingdom email: m.pignatari@hull.ac.uk The NuGrid collaboration (www.nugridstars.org)
Carolyn L. Doherty
Affiliation:
Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungarian Academy of Sciences, H-1121 Budapest, Hungary email: maria.lugaro@csfk.mta.hu, carolyn.doherty@csfk.mta.hu
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Abstract

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Planetary nebulae retain the signature of the nucleosynthesis and mixing events that occurred during the previous AGB phase. Observational signatures complement observations of AGB and post-AGB stars and their binary companions. The abundances of the elements heavier than iron such as Kr and Xe in planetary nebulae can be used to complement abundances of Sr/Y/Zr and Ba/La/Ce in AGB stars, respectively, to determine the operation of the slow neutron-capture process (the s process) in AGB stars. Additionally, observations of the Rb abundance in Type I planetary nebulae may allow us to infer the initial mass of the central star. Several noble gas components present in meteoritic stardust silicon carbide (SiC) grains are associated with implantation into the dust grains in the high-energy environment connected to the fast winds from the central stars during the planetary nebulae phase.

Keywords

nuclear reactionsnucleosynthesisabundancesstars: AGB and post-AGBstars: abundancesstars: chemically peculiar
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. 86 - 94
Copyright
Copyright © International Astronomical Union 2017 

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