The Radius and Entropy of a Magnetized, Rotating, Fully Convective Star: Analysis with Depth-dependent Mixing Length Theories (2018)
Attributed to:
From Molecular Clouds to Exoplanets
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aab3da
Publication URI: http://dx.doi.org/10.3847/1538-4357/aab3da
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2
ISSN: 15384357 0004637X