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Updated: Jul 5, 2026

Coulomb Explosion Imaging as a Tool to Distinguish Between Stereoisomers
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コメント on "3Heの深層混合:ビッグバンと恒星の核合成を調和させる"

Dana S Balser1, Robert T Rood, T M Bania

  • 1National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903-2475, USA. dbalser@nrao.edu

Science (New York, N.Y.)
|September 1, 2007
PubMed
まとめ

低質量恒星は,以前考えられていたように,すべてのヘリウム-3 (3He) を破壊しないかもしれません. 新しい発見は,一部の恒星が相当量の3Heを産生することを示唆し,既存の深層混合モデルに挑戦しています.

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