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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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Autores principales: Nicola Keaveney, Laura Boyle, Matt Redman
Formato: Artigo
Lenguaje:Inglês
Publicado: MDPI AG 2020-05-01
Colección:Galaxies
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Acceso en línea:https://www.mdpi.com/2075-4434/8/2/41
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