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Why the observed spin evolution of older-than-solar-like stars might not require a dynamo mode change (2023)

First Author: Kotorashvili K

Attributed to: Isaac Newton Institute for Mathematical Sciences funded by EPSRC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stad981

Publication URI: http://dx.doi.org/10.1093/mnras/stad981

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 1