Successive common envelope events from multiple planets
arXiv:2011.11106 · doi:10.1093/mnrasl/slab017
Abstract
Many stars harbour multi-planet systems. As these stars expand late in their evolutions, the innermost planet may be engulfed, leading to a common envelope (CE) event. Even if this is insufficient to eject the envelope, it may expand the star further, causing additional CE events, with the last one unbinding what remains of the envelope. This multi-planet CE scenario may have broad implications for stellar and planetary evolution across a range of systems. We develop a simplified version and show that it may be able to explain the recently observed planet WD 1856 b.
arXiv comment5 pages, 2 figures, accepted for publication in MNRAS Letters
References in corpus (36)
- Galactic Stellar and Substellar Initial Mass Function
- Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation
- Shrinking binary and planetary orbits by Kozai cycles with tidal friction
- Common Envelope Evolution: Where we stand and how we can move forward
- Planet Migration and Binary Companions: the case of HD 80606b
- Are There Unstable Planetary Systems Around White Dwarfs?
- The White Dwarf Initial-Final Mass Relation for Progenitor Stars From 0.85 to 7.5 M
- The Orbital Evolution of Gas Giant Planets around Giant Stars
- Accretion and diffusion in white dwarfs. New diffusion timescales and applications to GD362 and G29-38
- The accretion of planets and brown dwarfs by giant stars -- II. solar mass stars on the red giant branch
- Low-Mass Binary Induced Outflows from Asymptotic Giant Branch Stars
- The Great Escape: How Exoplanets and Smaller Bodies Desert Dying Stars
- On the Binding Energy Parameter of Common Envelope Evolution
- A Giant Planet Candidate Transiting a White Dwarf
- Accretion of a giant planet onto a white dwarf
- On the Orbits of Low-mass Companions to White Dwarfs and the Fates of the Known Exoplanets
- Constraints on the Lifetimes of Disks Resulting from Tidally Destroyed Rocky Planetary Bodies
- The Accretion of Brown Dwarfs and Planets by Giant Stars -- I. AGB Stars
- Oxygen fugacities of extrasolar rocks: Evidence for an Earth-like geochemistry of exoplanets
- Tides and Tidal Engulfment in Post-Main Sequence Binaries: Period Gaps for Planets and Brown Dwarfs Around White Dwarfs
- Accretion in common envelope evolution
- The formation of high-field magnetic white dwarfs from common envelopes
- Hydrodynamic Simulations of the Interaction between Giant Stars and Planets
- Episodic mass ejections from common-envelope objects
- Runaway Coalescence at the Onset of Common Envelope Episodes
- WD 1856 b: a close giant planet around a white dwarf that could have survived a common-envelope phase
- The Role of Convection in Determining the Ejection Efficiency of Common Envelope Interactions
- Enhanced Lidov-Kozai migration and the formation of the transiting giant planet WD1856+534b
- Kozai Migration Naturally Explains the White Dwarf Planet WD1856b
- The lifetimes of planetary debris discs around white dwarfs
- Wind-accelerated orbital evolution in binary systems with giant stars
- How Drag Force Evolves in Global Common Envelope Simulations
- Convection and Spin-Up During Common Envelope Evolution: The Formation of Short-Period Double White Dwarfs
- Common Envelope Evolution on the Asymptotic Giant Branch: Unbinding within a Decade?
- Dynamical evolution of two-planet systems and its connection with white dwarf atmospheric pollution
- Hydrodynamic Simulations of Disrupted Planetary Accretion Discs Inside the Core of an AGB Star
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- Close detached white dwarf + brown dwarf binaries: further evidence for low values of the common envelope efficiency
- Giant planet engulfment by evolved giant stars: light curves, asteroseismology, and survivability
- A red giant branch common envelope evolution scenario for the exoplanet WD 1856 b
- Can Gaia find planets around white dwarfs?
- The smallest planetary drivers of white dwarf pollution
- Gemini/GMOS Transmission Spectroscopy of the Grazing Planet Candidate WD 1856+534 b
- The future influence of six exoplanets on the envelope properties of their parent stars on the giant branches
- TTV Constraints on Additional Planets in the WD 1856+534 system
- Lost in space: companions' fatal dance around massive dying stars
- High-resolution resonant portraits of a single-planet white dwarf system
- Rapid expansion of red giant stars during core helium flash by waves propagation to the envelope and implications to exoplanets
- Common envelope evolution and triple dynamics as potential pathways to form the inner white dwarf + brown dwarf binary of the triple star system Gaia 0007-1605
- Residual eccentricity of an Earth-like planet orbiting a red giant Sun
- Second-generation planet formation after tidal disruption from common envelope evolution
- Fates of the sub-stellar objects (FOSSO) I. Fates of the known brown dwarfs in main-sequence--BD binaries
- Atmospheric Signatures of Common Envelope Evolution in White Dwarf Planets
- Faint intermediate luminosity optical transients (ILOTs) from engulfing exoplanets on the Hertzsprung gap
- Life in the dark: Potential urability of moons of rogue planets