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Why the observed spin evolution of older-than-solar-like stars might not require a dynamo mode change

Kotorashvili, K., Blackman, E. G., & Owen, J. E. (2023). Why the observed spin evolution of older-than-solar-like stars might not require a dynamo mode change. In Monthly Notices of the Royal Astronomical Society (Vol. 522, Issue 1, pp. 1583–1590). Oxford University Press (OUP). https://doi.org/10.1093/mnras/stad981

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