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Laboratory gas phase spectroscopy of carbon molecular structures in relation to diffuse interstellar bands

机译:与弥散星际带有关的碳分子结构的实验室气相色谱

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摘要

An experiment suitable for studying the carbon molecular structures which are the candidates for carriers of the diffuse interstellar bands (DIBs) in astrophysical spectra has been developed in the plasma-chemistry laboratory of the Masaryk University in Brno. The experimental arrangement including an apparatus for detecting the gas phase spectra Of monopolar high-frequency discharge is described. The preliminary results involving a Search for the ultraviolet, visible, and near-infrared well pronounced features of the carbon Molecular structures are discussed.
机译:在布尔诺的马萨里克大学的等离子体化学实验室中,开展了一项适合研究碳分子结构的实验,该碳分子结构是天体物理光谱中弥散星际带(DIB)的载体。描述了包括用于检测单极高频放电的气相谱的设备的实验装置。讨论了初步结果,包括寻找碳分子结构的紫外线,可见光和近红外光的明显特征。

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