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Why the observed spin evolution of older-than-solar-like st..:
Kotorashvili, Ketevan
;
Blackman, Eric G
;
Owen, James E
Monthly Notices of the Royal Astronomical Society. 522 (2023) 1 - p. 1583-1590 , 2023
Link:
https://doi.org/10.1093/mnras/stad981
RT Journal T1 <Title>Why the observed spin evolution of older-than-solar-like stars might not require a dynamo mode change</Title> UL https://suche.suub.uni-bremen.de/peid=cr-10.1093_mnras_stad981&Exemplar=1&LAN=DE A1 Kotorashvili, Ketevan A1 Blackman, Eric G A1 Owen, James E PB Oxford University Press (OUP) YR 2023 SN 0035-8711 SN 1365-2966 JF Monthly Notices of the Royal Astronomical Society VO 522 IS 1 SP 1583 OP 1590 LK http://dx.doi.org/https://doi.org/10.1093/mnras/stad981 DO https://doi.org/10.1093/mnras/stad981 SF ELIB - SuUB Bremen
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