3D hydro simulations demonstrate that donor central concentration (ρ_c/ρ_bar) controls inspiral morphology and mass-ejection history in common-envelope events for luminous red novae.
N., Covarrubias, R., & Ramirez-Ruiz, E
3 Pith papers cite this work, alongside 1 external citations. Polarity classification is still indexing.
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Accretion laws with super-linear mass dependence produce divergent population evolution that broadens compact-object mass distributions and drives binary mass ratios toward unity, providing a pathway to massive gravitational-wave sources.
TOI-5882, a lithium-enriched subgiant with a brown dwarf companion, shows enrichment consistent with engulfment of a super-Earth to Neptune-mass planet.
citing papers explorer
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Hydrodynamic Response of Mildly Evolved Common Envelope Donors in Luminous Red Novae
3D hydro simulations demonstrate that donor central concentration (ρ_c/ρ_bar) controls inspiral morphology and mass-ejection history in common-envelope events for luminous red novae.
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Accretion-Driven Evolution of Compact-Object Populations in Gas-Rich Environments and the Origin of Massive Gravitational-Wave Sources
Accretion laws with super-linear mass dependence produce divergent population evolution that broadens compact-object mass distributions and drives binary mass ratios toward unity, providing a pathway to massive gravitational-wave sources.
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Lithium Enrichment in a Subgiant Star with a Brown Dwarf Companion: A Planetary Engulfment Candidate
TOI-5882, a lithium-enriched subgiant with a brown dwarf companion, shows enrichment consistent with engulfment of a super-Earth to Neptune-mass planet.