Flaring Activity for Low-mass Stars in the β Pictoris Moving Group

Stellar flares from K and M dwarfs release panchromatic radiation characterized by a significantly higher brightness temperature (∼9–20 kK) than the star. The increased frequency of magnetic activity on young low-mass stars results in the energy released during flaring events becoming a notable cont...

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Hlavní autoři:	Jordan N. Ealy, Joshua E. Schlieder, Thaddeus D. Komacek, Emily A. Gilbert
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2024-01-01
Edice:	The Astronomical Journal
Témata:	Optical flares Stellar flares Exoplanets M dwarf stars K dwarf stars Red dwarf flare stars
On-line přístup:	https://doi.org/10.3847/1538-3881/ad6b7e
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