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Updated: Jun 26, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
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恒星形成の過程における複数の長さスケールの自己重力の役割

Alyssa A Goodman1, Erik W Rosolowsky, Michelle A Borkin

  • 1Initiative in Innovative Computing at Harvard, Cambridge, Massachusetts 02138, USA. agoodman@cfa.harvard.edu

Nature
|January 6, 2009
PubMed
まとめ

自己重力は,分子雲の中で星が形成されるのに極めて重要です. L1448雲の分析は,自己重力が様々なスケール,特に星前核の星形成に大きく影響することを示しています.

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