Romanini D, Biennier L, Salama F, Kachanov A, Allamandola L J, Stoeckel F
Laboratoire de Spectrometrie Physique, Universite J. Fourier, Grenoble, France.
Chem Phys Lett. 1999 Apr 2;303(1-2):165-70. doi: 10.1016/s0009-2614(99)00210-9.
Naphthalene cations (C10H+8) were produced in a slit jet coupled with an electronic discharge, and cavity ring down was used to obtain its absorption spectrum in the region 645-680 nm. Two of the strongest C10H+8 bands previously characterized by matrix isolation spectroscopy were found, both with a fractional blue shift of about 0.5%. This is the first gas-phase electronic absorption spectrum of an ionized polycyclic aromatic hydrocarbon (PAH). This work opens the way for a direct comparison of laboratory PAH spectra with the diffuse interstellar bands (DIB), the origin of which still constitutes an open problem in astrophysics.
萘阳离子(C10H+8)通过与电子放电耦合的狭缝射流产生,并利用腔衰荡技术获得其在645 - 680 nm区域的吸收光谱。发现了两个先前通过基质隔离光谱表征的最强C10H+8谱带,两者均有大约0.5%的蓝移。这是离子化多环芳烃(PAH)的首个气相电子吸收光谱。这项工作为将实验室PAH光谱与弥漫星际带(DIB)进行直接比较开辟了道路,弥漫星际带的起源在天体物理学中仍然是一个悬而未决的问题。