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Updated: May 5, 2026

Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry
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ケルビン・ヘルムホルツの不安定性は,新星爆発における不均質な混合の源である

Jordi Casanova1, Jordi José, Enrique García-Berro

  • 1Departament de Física i Enginyeria Nuclear, EUETIB, Universitat Politècnica de Catalunya, E-08036 Barcelona, Spain.

Nature
|October 21, 2011
PubMed
まとめ

古典的な新星は濃縮ガスを放出するが,混合は説明がつかないままだった. 立体シミュレーションでは,浮遊する指のドライブが混ざり合っていることが明らかになり,噴出された新星殻の化学的不均一性が説明されます.

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