X-Ray, UV, and Optical Observations of Proxima Centauri’s Stellar Cycle

Proxima Cen (GJ 551; dM5.5e) is one of only about a dozen fully convective stars known to have a stellar cycle, and the only one to have long-term X-ray monitoring. A previous analysis found that X-ray and mid-UV observations, particularly two epochs of data from Swift, were consistent with a well-s...

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Үндсэн зохиолчид:	Bradford J. Wargelin, Steven H. Saar, Zackery A. Irving, Jonathan D. Slavin, Peter Ratzlaff, José-Dias do Nascimento Jr
Формат:	Artigo
Хэл сонгох:	Inglês
Хэвлэсэн:	IOP Publishing 2024-01-01
Цуврал:	The Astrophysical Journal
Нөхцлүүд:	Stellar activity Late-type dwarf stars M dwarf stars
Онлайн хандалт:	https://doi.org/10.3847/1538-4357/ad8faa
Шошгууд:	Шошго нэмэх Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!