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Updated: Apr 18, 2026

Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions
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低質量恒星の重元素合成の温度と年代順

P Neyskens1, S Van Eck1, A Jorissen1

  • 1Institut d'Astronomie et d'Astrophysique, Université libre de Bruxelles (ULB), CP 226, 1050 Bruxelles, Belgium.

Nature
|January 9, 2015
PubMed
まとめ

この研究では,進化した恒星のゆっくりとした中性子捕獲プロセス (sプロセス) の温度を決定し,炭素13を主要な中性子源として支持しました. この発見は,星における重元素合成の時間スケールも提供している.

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