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Updated: Aug 14, 2026

Digital Inline Holographic Microscopy (DIHM) of Weakly-scattering Subjects
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Cygnus OB2 No. に向かって拡散した恒星間介質でH3+の検出 12 12 12 12 12 12 12 12 12 12 12 12 12 12 12 12 12 12 12 12 12 12 12 12 12 12 12

B J McCall1, T R Geballe, K H Hinkle

  • 1Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637, USA.

Science (New York, N.Y.)
|April 16, 1998
PubMed
まとめ

どこにでも存在する三水素カチオン (H3+) は,星間化学の鍵です. 拡散した星間媒介で最近検出されたことは,高い濃度ではなく,長い吸収経路が,その密度を説明することを示唆しています.

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