The Diffuse Interstellar Bands in History and in the UV

T. Snow, J. D. Destree
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引用次数: 2

Abstract

The diffuse interstellar bands (DIBs) have been known of since 1922, but their carrier molecules remain unidentified to this day. We present a brief history of DIB observations, followed by a list of constraints any suggested origin must face, and finally a preview of current research for ultraviolet DIBs using the Cosmic Origins Spectrograph on the Hubble Space Telescope . We conclude that PAHs are consistent with all the listed constraints, but that PAHs may not be the only molecular species responsible for the DIBs.
历史上的漫射星际带和紫外线
弥漫星际带(DIBs)自1922年以来就已为人所知,但它们的载体分子至今仍未被识别。我们简要介绍了DIB观测的历史,然后列出了任何提出的起源必须面对的约束条件,最后是使用哈勃太空望远镜上的宇宙起源光谱仪对紫外DIB的当前研究的预览。我们得出结论,多环芳烃符合所有列出的约束条件,但多环芳烃可能不是唯一负责dib的分子物种。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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