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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/10.48550/arxiv.2301.04693

Publication URI: https://arxiv.org/abs/2301.04693

Type: Other