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Updated: Feb 16, 2026

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脈動する白矮星の地震地図から見た,酸素が多く存在する大きな核

N Giammichele1,2, S Charpinet1, G Fontaine2

  • 1Institut de Recherche en Astrophysique et Planétologie (IRAP), Université de Toulouse, Centre National de la Recherche Scientifique (CNRS), UPS, Centre National d'Études Spatiales (CNES), 14 Avenue Edouard Belin, F-31400 Toulouse, France.

Nature
|January 9, 2018
PubMed
まとめ

ホワイト・ダワーフ・スターは 恒星の進化の秘密を明らかにします KIC08626021のアステロシズモロジーは,その酸素の核が現在のモデルが予測するよりも大きく,より酸素が豊富であることを示し,恒星の進化理論に挑戦しています.

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