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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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是一个类似于烯的分子离子导致了4430安格斯特罗姆的分散星际吸收带吗?

F Salama1, L J Allamandola

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

Nature
|July 2, 1992
PubMed
概括

分散星际带 (DIB) 是天文吸收特征. 实验室测量表明,酸可能是特定DIB的原因,这可能解释了多环芳碳化合物如何处理星际光.

关键词:
美国宇航局中心ARC中心美国宇航局的学科是外生态学.

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