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Autor:
Alejandro Núñez, Marcel A. Agüeros, Jason L. Curtis, Kevin R. Covey, Stephanie T. Douglas, Sabine R. Chu, Stanislav DeLaurentiis, Minzhi (Luna) Wang, Jeremy J. Drake
Publikováno v:
The Astrophysical Journal, Vol 962, Iss 1, p 12 (2024)
Low-mass (≲1.2 M _⊙ ) main-sequence stars lose angular momentum over time, leading to a decrease in their magnetic activity. The details of this rotation–activity relation remain poorly understood, however. Using observations of members of the
Externí odkaz:
https://doaj.org/article/92ceda790eba4c13a4b1ba6152c5a793
