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Updated: Jul 15, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
11:20

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Published on: July 2, 2012

桜井のオブジェクトのリアルタイムの恒星進化

Marcin Hajduk1, Albert A Zijlstra, Falk Herwig

  • 1School of Physics and Astronomy, University of Manchester, Post Office Box 88, Manchester M60 1QD, UK.

Science (New York, N.Y.)
|April 12, 2005
PubMed
まとめ

白い矮星の恒星のヘリウム再燃は,急速な冷却と質量放出を引き起こす可能性があります. 新しいモデルは,この急速な進化を説明し,観測により,予測された再加熱と炭素塵の発生の可能性が確認されています.

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