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Laboratory spectra of cold gas phase polycyclic aromatic hydrocarbon cations, and their possible relation to the diffuse interstellar bands

机译:冷气相多环芳烃阳离子的实验室光谱及其与星际扩散带的可能关系

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A novel laboratory technique is described, combining the use of supersonic expansion, laser excitation and small aromatic-rare gas van der Waals (vdW) clusters properties, which was developed to access the electronic absorption spectra of the polycyclic aromatic hydrocarbon (PAH) cations in the visible. It consists in preparing vdW complexes of the PAH molecule with a rare gas in a molecular beam, to photoionize it by resonant selective two-photon ionization, then to photodissociate this ionic complex by means of a delayed laser pulse in a time-of-flight mass spectrometer. The method is illustrated by presenting the visible spectra of the Naphthalene, Phenanthrene, Fluorene and Phenylacetylene cations. Such spectra can be unambiguously compared to the astronomical spectra of reddened stars, which exhibit the so-called diffuse interstellar bands (DIBs) in absorption. An interesting feature of the technique is its ability to measure the absolute absorption cross-sections. The large values of the oscillator strengths of the transitions, which are derived, are discussed in the astrophysical context which consists in considering that the PAH cations could be carriers for some of the DIBs. (C) 2001 Elsevier Science B.V. All rights reserved. [References: 45]
机译:描述了一种新颖的实验室技术,该技术结合了超音速膨胀,激光激发和小型芳香族稀有范德华(vdW)团簇性质的使用,该性质被开发用于访问多环芳烃(PAH)阳离子的电子吸收光谱。可见的。它包括用分子束中的稀有气体制备PAH分子的vdW络合物,通过共振选择性双光子电离使其电离,然后通过延迟的激光脉冲在飞行时间对该离子络合物进行光离解。质谱仪。通过呈现萘,菲,芴和苯乙炔阳离子的可见光谱来说明该方法。可以将此类光谱与变红的恒星的天文光谱进行明确比较,该变红的恒星在吸收中表现出所谓的弥漫星际带(DIB)。该技术的一个有趣特征是它能够测量绝对吸收截面。在天体物理学的背景下讨论了导出的跃迁的振荡器强度的较大值,其中包括考虑到PAH阳离子可能是某些DIB的载流子。 (C)2001 Elsevier Science B.V.保留所有权利。 [参考:45]

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