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Updated: Jul 12, 2025

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JWSTによって観測されたコンパクトオブジェクトの融合における重元素の生成

Andrew J Levan1,2, Benjamin P Gompertz3,4, Om Sharan Salafia5,6

  • 1Department of Astrophysics, Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud University, Nijmegen, The Netherlands. a.levan@astro.ru.nl.

Nature
|October 25, 2023
PubMed
まとめ

明るいガンマ線爆発 (GRB) の観測により,重元素の生成を示したキロノヴァが発見された. ジェームズ・ウェブ宇宙望遠鏡はテルリウムとランタノイドを検出し,GRBは多様なrプロセス元素を生成することを確認しました.

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