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.
Title resolution pending
1 Pith paper cite this work, alongside 19 external citations. Polarity classification is still indexing.
1
Pith paper citing it
19
external citations · OpenAlex
citation-role summary
background 1
citation-polarity summary
fields
astro-ph.SR 1years
2025 1verdicts
CONDITIONAL 1roles
background 1polarities
unclear 1representative citing papers
citing papers explorer
-
Simulations of Flare Chemistry in Brown Dwarf Companions to Active M Dwarfs
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.