Neutron-Capture Element Abundances in Planetary Nebulae

Nebular spectroscopy is a valuable tool for assessing the production of heavy elements by slow neutron(<i>n</i>)-capture nucleosynthesis (the <i>s</i>-process). Several transitions of <i>n</i>-capture elements have been identified in planetary nebulae (PNe) in the...

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Main Author: N. C. Sterling
Format: Article
Language:English
Published: MDPI AG 2020-06-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/8/2/50
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author N. C. Sterling
author_facet N. C. Sterling
author_sort N. C. Sterling
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description Nebular spectroscopy is a valuable tool for assessing the production of heavy elements by slow neutron(<i>n</i>)-capture nucleosynthesis (the <i>s</i>-process). Several transitions of <i>n</i>-capture elements have been identified in planetary nebulae (PNe) in the last few years, with the aid of sensitive, high-resolution, near-infrared spectrometers. Combined with optical spectroscopy, the newly discovered near-infrared lines enable more accurate abundance determinations than previously possible, and provide access to elements that had not previously been studied in PNe or their progenitors. Neutron-capture elements have also been detected in PNe in the Sagittarius Dwarf galaxy and in the Magellanic Clouds. In this brief review, I discuss developments in observational studies of <i>s</i>-process enrichments in PNe, with an emphasis on the last five years, and note some open questions and preliminary trends.
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spelling doaj.art-b05d80edc796458283110f3d4ed8a5f72023-11-20T04:03:25ZengMDPI AGGalaxies2075-44342020-06-01825010.3390/galaxies8020050Neutron-Capture Element Abundances in Planetary NebulaeN. C. Sterling0Department of Physics, University of West Georgia, Carrollton, GA 30118, USANebular spectroscopy is a valuable tool for assessing the production of heavy elements by slow neutron(<i>n</i>)-capture nucleosynthesis (the <i>s</i>-process). Several transitions of <i>n</i>-capture elements have been identified in planetary nebulae (PNe) in the last few years, with the aid of sensitive, high-resolution, near-infrared spectrometers. Combined with optical spectroscopy, the newly discovered near-infrared lines enable more accurate abundance determinations than previously possible, and provide access to elements that had not previously been studied in PNe or their progenitors. Neutron-capture elements have also been detected in PNe in the Sagittarius Dwarf galaxy and in the Magellanic Clouds. In this brief review, I discuss developments in observational studies of <i>s</i>-process enrichments in PNe, with an emphasis on the last five years, and note some open questions and preliminary trends.https://www.mdpi.com/2075-4434/8/2/50planetary nebulae, generalnuclear reactions, nucleosynthesis, abundancesstarsAGB and post-AGBinfrared, general
spellingShingle N. C. Sterling
Neutron-Capture Element Abundances in Planetary Nebulae
Galaxies
planetary nebulae, general
nuclear reactions, nucleosynthesis, abundances
stars
AGB and post-AGB
infrared, general
title Neutron-Capture Element Abundances in Planetary Nebulae
title_full Neutron-Capture Element Abundances in Planetary Nebulae
title_fullStr Neutron-Capture Element Abundances in Planetary Nebulae
title_full_unstemmed Neutron-Capture Element Abundances in Planetary Nebulae
title_short Neutron-Capture Element Abundances in Planetary Nebulae
title_sort neutron capture element abundances in planetary nebulae
topic planetary nebulae, general
nuclear reactions, nucleosynthesis, abundances
stars
AGB and post-AGB
infrared, general
url https://www.mdpi.com/2075-4434/8/2/50
work_keys_str_mv AT ncsterling neutroncaptureelementabundancesinplanetarynebulae