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Updated: May 5, 2026

Quantification of Hydrogen Concentrations in Surface and Interface Layers and Bulk Materials through Depth Profiling with Nuclear Reaction Analysis
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HD 209458bbの周りの高速水素の説明としてエネルギー中性原子

M Holmström1, A Ekenbäck, F Selsis

  • 1Swedish Institute of Space Physics, PO Box 812, SE-98128 Kiruna, Sweden. matsh@irf.se

Nature
|February 22, 2008
PubMed
まとめ

恒星系外惑星HD 209458bの周りの高速水素は,放射線圧だけでなく,恒星風の相互作用によって説明されます. この発見は,系外惑星の近くの恒星風を研究するための新しい方法を提供します.

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