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Updated: Jul 8, 2026

Bringing the Visible Universe into Focus with Robo-AO
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ルビジアムに富むアシンプトティックな巨大な支柱星である

D A García-Hernández1, P García-Lario, B Plez

  • 1ISO Data Centre, European Space Astronomy Centre, Research and Scientific Support Department, European Space Agency, Villafranca del Castillo, Apdo. 50727, E-28080 Madrid, Spain. agarcia@astro.as.utexas.edu

Science (New York, N.Y.)
|November 11, 2006
PubMed
まとめ

天文学者はルビジアムに富んだ恒星を発見し, (22) Ne (((alpha,n) (((25) Mg反応がアシンプトティック・ジャイアント・ブランチ (AGB) 恒星における主要な中性子源であるという証拠を提供した. この発見は,恒星の進化と太陽系の初期状態に関する私たちの理解に影響を与えます.

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