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Kotorashvili, K · 2024 · arXiv (Cornell University) · DOI 10.48550/arxiv.2411.17916 · arXiv 2411.17916

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astro-ph.SR 1

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2025 1

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CONDITIONAL 1

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Simulations of Flare Chemistry in Brown Dwarf Companions to Active M Dwarfs

astro-ph.SR · 2025-09-08 · conditional · novelty 6.0

Superflares from M dwarf hosts drive order-of-magnitude atmospheric chemistry changes in brown dwarf companions, but fast chemical relaxation (under a day) leaves high-resolution emission spectroscopy within hours of a flare as the only plausible, still very challenging, detection route.

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  • Simulations of Flare Chemistry in Brown Dwarf Companions to Active M Dwarfs astro-ph.SR · 2025-09-08 · conditional · none · ref 23

    Superflares from M dwarf hosts drive order-of-magnitude atmospheric chemistry changes in brown dwarf companions, but fast chemical relaxation (under a day) leaves high-resolution emission spectroscopy within hours of a flare as the only plausible, still very challenging, detection route.