Giant Planet Engulfment by Evolved Giant Stars: Light Curves, Asteroseismology, and Survivability
About ten percent of Sun-like (1–2 M _⊙ ) stars will engulf a 1–10 M _J planet as they expand during the red giant branch (RGB) or asymptotic giant branch (AGB) phase of their evolution. Once engulfed, these planets experience a strong drag force in the star’s convective envelope and spiral inward,...
Main Authors: | Christopher E. O’Connor, Lars Bildsten, Matteo Cantiello, Dong Lai |
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Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
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Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/acd2d4 |
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