Published November 9, 2022 | Version v1
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Supplmental Material to Nature of Intense Magnetism and Differential Rotation In Convective Dynamos of M-Dwarf Stars With Tachoclines

Authors/Creators

  • 1. University of Colorado Boulder

Description

Inlists and source files used for the MESA model in the paper "Nature of Intense Magnetism and Differential Rotation In Convective Dynamos of M-Dwarf Stars With Tachoclines"

This work employed MESA version 10398.

Files

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