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