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Updated: May 6, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
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初期の恒星形成の低質量残骸である

R Schneider1, A Ferrara, R Salvaterra

  • 1Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, 50125 Firenze, Italy.

Nature
|April 25, 2003
PubMed
まとめ

初期の恒星は金属なしで形成され,大質量恒星に好意を示した. しかし,金属度が極めて低いガス中の塵は,今日の質量が低い星の形成を可能にした.

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