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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MDPI AG
2020-06-01
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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 |
collection | DOAJ |
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. |
first_indexed | 2024-03-10T19:07:22Z |
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id | doaj.art-b05d80edc796458283110f3d4ed8a5f7 |
institution | Directory Open Access Journal |
issn | 2075-4434 |
language | English |
last_indexed | 2024-03-10T19:07:22Z |
publishDate | 2020-06-01 |
publisher | MDPI AG |
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series | Galaxies |
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 |