Answers are grounded in this paper and cite their sources.
Context. Interpretation of interferometric observations of rapidly rotating stars requires a good model of their surface effective temperature. Until now, laws of the form have been used, but they are only valid for slowly rotating stars.
No takes yet. Share an insight, caveat, or question.
Lara et al. (2011) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: