Role of Nonthermal Processes in the Quiescent and Active Millimeter Spectrum of a Young M Dwarf

Millimeter (mm) emission from F-M dwarfs (cool stars) primarily traces chromospheric activity, with thermal emission thought to dominate in quiescence. Despite the high chromospheric activity, the quiescent mm spectral fluence (mm- S ( ν )) of young (<1 Gyr) M dwarfs (dMs) remains largely unexplored...

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Autors principals:	Atul Mohan, Peter H. Hauschildt, Birgit Fuhrmeister, Surajit Mondal, Vladimir Airapetian, Sven Wedemeyer
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2025-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Red dwarf flare stars Stellar activity Millimeter astronomy Stellar chromospheres Stellar coronae Stellar atmospheres
Accés en línia:	https://doi.org/10.3847/1538-4357/ade9bf
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