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Updated: Oct 2, 2025

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球状星群における反復的な高速電波源

F Kirsten1,2, B Marcote3, K Nimmo4,5

  • 1Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory, Onsala, Sweden. kirsten@astron.nl.

Nature
|February 24, 2022
PubMed
まとめ

球状星団に局限した高速電波 (FRB) は,既存のモデルに挑戦しています. この発見は,FRBは,白矮星の崩壊や,これらの密度の高い恒星環境内の二重結合によって形成された中性子星から生じる可能性があることを示唆しています.

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