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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Main Authors: Nicola Keaveney, Laura Boyle, Matt Redman
Format: Article
Language:English
Published: MDPI AG 2020-05-01
Series:Galaxies
Subjects:
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.
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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