On the Structure and Properties of Differentially Rotating, Main-Sequence Stars in the 1-2 M☉ Range

@article{Macgregor2007OnTS,
  title={On the Structure and Properties of Differentially Rotating, Main-Sequence Stars in the 1-2 M☉ Range},
  author={Keith B. Macgregor and Stephen Jackson and Andrew Skumanich and Travis S. Metcalfe},
  journal={The Astrophysical Journal},
  year={2007},
  volume={663},
  pages={560-572}
}
We present models for chemically homogeneous, differentially rotating, main-sequence stars with masses in the range 1-2 M☉. The models were constructed using a code based on a reformulation of the self-consistent field method of computing the equilibrium stellar structure for a specified conservative internal rotation law. Relative to nonrotating stars of the same mass, these models all have reduced luminosities and effective temperatures, and flattened photospheric shapes (i.e., decreased… 

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