A Census of Near-UV M-dwarf Flares Using Archival GALEX Data and the gPHOTON2 Pipeline

M-dwarfs are common stellar hosts of habitable-zone exoplanets. Near-UV (NUV) radiation can severely impact the atmospheric and surface conditions of such planets, making the characterization of NUV flaring activity a key aspect in determining habitability. We use archival data from the Galaxy Evolu...

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Hlavní autoři:	Param Rekhi, Sagi Ben-Ami, Volker Perdelwitz, Yossi Shvartzvald
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2023-01-01
Edice:	The Astrophysical Journal
Témata:	Red dwarf flare stars Stellar flares M dwarf stars Ultraviolet astronomy Near ultraviolet astronomy Habitable planets
On-line přístup:	https://doi.org/10.3847/1538-4357/ace5ac
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