Shaping of Planetary Nebulae by Exoplanets
(1) Background: We investigate the hypothesis that exoplanet engulfment can help explain the observed non-spherical planetary nebula population, as a complementary shaping mechanism to the binary hypothesis. The aim is to investigate the extent to which massive planets can explain the population of...
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Format: | Article |
Language: | English |
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MDPI AG
2020-05-01
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Series: | Galaxies |
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Online Access: | https://www.mdpi.com/2075-4434/8/2/41 |
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author | Nicola Keaveney Laura Boyle Matt Redman |
author_facet | Nicola Keaveney Laura Boyle Matt Redman |
author_sort | Nicola Keaveney |
collection | DOAJ |
description | (1) Background: We investigate the hypothesis that exoplanet engulfment can help explain the observed non-spherical planetary nebula population, as a complementary shaping mechanism to the binary hypothesis. The aim is to investigate the extent to which massive planets can explain the population of non-spherical planetary nebulae; (2) Methods: This research utilises a new tool to calculate the planet-fraction of planetary nebulae progenitor stars called <span style="font-variant: small-caps;">simsplash</span>; (3) Results: we conclude that ∼15–30% of non-spherical planetary nebulae around single stars will have a history in which they engulfed a massive planet on the AGB; and (4) Conclusions: Engulfment of massive exoplanets may contribute significantly to the formation of non-spherical planetary nebulae around single stars, yet appears to be insufficient to explain them all. |
first_indexed | 2024-03-10T19:49:46Z |
format | Article |
id | doaj.art-8a215fad747a4cc286d8ed560d4dcace |
institution | Directory Open Access Journal |
issn | 2075-4434 |
language | English |
last_indexed | 2024-03-10T19:49:46Z |
publishDate | 2020-05-01 |
publisher | MDPI AG |
record_format | Article |
series | Galaxies |
spelling | doaj.art-8a215fad747a4cc286d8ed560d4dcace2023-11-20T00:29:52ZengMDPI AGGalaxies2075-44342020-05-01824110.3390/galaxies8020041Shaping of Planetary Nebulae by ExoplanetsNicola Keaveney0Laura Boyle1Matt Redman2National University of Ireland Galway, University Rd, H91 TK33 Galway, IrelandNational University of Ireland Galway, University Rd, H91 TK33 Galway, IrelandNational University of Ireland Galway, University Rd, H91 TK33 Galway, Ireland(1) Background: We investigate the hypothesis that exoplanet engulfment can help explain the observed non-spherical planetary nebula population, as a complementary shaping mechanism to the binary hypothesis. The aim is to investigate the extent to which massive planets can explain the population of non-spherical planetary nebulae; (2) Methods: This research utilises a new tool to calculate the planet-fraction of planetary nebulae progenitor stars called <span style="font-variant: small-caps;">simsplash</span>; (3) Results: we conclude that ∼15–30% of non-spherical planetary nebulae around single stars will have a history in which they engulfed a massive planet on the AGB; and (4) Conclusions: Engulfment of massive exoplanets may contribute significantly to the formation of non-spherical planetary nebulae around single stars, yet appears to be insufficient to explain them all.https://www.mdpi.com/2075-4434/8/2/41planetary nebulaeplanet engulfmentexoplanets |
spellingShingle | Nicola Keaveney Laura Boyle Matt Redman Shaping of Planetary Nebulae by Exoplanets Galaxies planetary nebulae planet engulfment exoplanets |
title | Shaping of Planetary Nebulae by Exoplanets |
title_full | Shaping of Planetary Nebulae by Exoplanets |
title_fullStr | Shaping of Planetary Nebulae by Exoplanets |
title_full_unstemmed | Shaping of Planetary Nebulae by Exoplanets |
title_short | Shaping of Planetary Nebulae by Exoplanets |
title_sort | shaping of planetary nebulae by exoplanets |
topic | planetary nebulae planet engulfment exoplanets |
url | https://www.mdpi.com/2075-4434/8/2/41 |
work_keys_str_mv | AT nicolakeaveney shapingofplanetarynebulaebyexoplanets AT lauraboyle shapingofplanetarynebulaebyexoplanets AT mattredman shapingofplanetarynebulaebyexoplanets |