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Updated: May 26, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability
06:42

Magnetically Induced Rotating Rayleigh-Taylor Instability

Published on: March 3, 2017

赤い巨星の核の急速な回転は,重力が支配する混合モードによって明らかにされています

Paul G Beck1, Josefina Montalban, Thomas Kallinger

  • 1Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, 3001 Leuven, Belgium. paul.beck@ster.kuleuven.be

Nature
|December 14, 2011
PubMed
まとめ

赤い巨星は,表面よりも速く回転する核を持っています. この研究では,恒星の振動モードを使用して,回転プロフィールの急な傾斜を明らかにし,恒星の内部に関する理論的予測を確認しました.

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