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Updated: Jul 18, 2026

Experimental Methods for Spin- and Angle-Resolved Photoemission Spectroscopy Combined with Polarization-Variable Laser
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Experimental Methods for Spin- and Angle-Resolved Photoemission Spectroscopy Combined with Polarization-Variable Laser

Published on: June 28, 2018

4,430アングストロムの星間吸収帯の原因はピレンのような分子イオンでしょうか?

F Salama1, L J Allamandola

  • 1NASA-Ames Research Center, Space Science Division, Moffett Field, California 94035, USA.

Nature
|July 2, 1992
PubMed
まとめ

拡散星間帯 (DIB) は,天文学的吸収特征である. 実験室での測定は,ピレンカチオンが特定のDIBの原因である可能性を示唆し,ポリサイクル芳香炭化水素が星間光をどのように処理するかを説明する可能性がある.

キーワード:
NASA Center ARCは,NASAセンターのARCとして運営されています.NASAの規律 エクゾバイオロジー

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