,

S Maret1, E A Bergin, C J Lada

  • 1Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, Michigan 48109-1042, USA. smaret@umich.edu

Nature
|July 28, 2006
PubMed
まとめ

恒星間窒素の大部分は原子であり,分子 (N2) ではない. これは,彗星の低N2と隕石や塵の窒素異常を説明し,宇宙窒素に関する以前の仮定に異議を唱える.

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