Gas-phase infrared spectrum of the coronene cation

被引:63
作者
Oomens, J
Sartakov, BG
Tielens, AGGM
Meijer, G
von Helden, G
机构
[1] FOM, Inst Plasma Phys Rijnhuizen, NL-3439 MN Nieuwegein, Netherlands
[2] Gen Phys Inst RAS, Moscow 119991, Russia
[3] Univ Groningen, Kapteyn Inst, Space Res Org Netherland, NL-9700 AV Groningen, Netherlands
[4] Univ Nijmegen, Dept Mol & Laser Phys, NL-6500 GL Nijmegen, Netherlands
关键词
infrared : ISM; ISM : molecules; methods : laboratory; techniques : spectroscopic;
D O I
10.1086/324170
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The gas-phase infrared spectrum of the coronene cation in the 700-1700 cm(-1) range is presented. The spectrum is obtained via multiphoton dissociation spectroscopy of ionic coronene stored in a quadrupole ion trap using the intense and narrowband infrared radiation of a free electron laser. The spectrum shows main absorption peaks at 849, 1327, and 1533 cm(-1) along with some weak and barely resolved features, in good agreement with density functional calculations if the effects of vibrational anharmonicity are accounted for. Relative line intensities show remarkable differences with respect to matrix isolation data. The novel experimental technique applied here leads in a natural way to an absorption spectrum of highly excited species. Hence, measured absorption spectra can be compared rather directly to interstellar emission spectra, negating to some extent the need for detailed model calculations.
引用
收藏
页码:L99 / L103
页数:5
相关论文
共 41 条
[1]   Modeling the unidentified infrared emission with combinations of polycyclic aromatic hydrocarbons [J].
Allamandola, LJ ;
Hudgins, DM ;
Sandford, SA .
ASTROPHYSICAL JOURNAL, 1999, 511 (02) :L115-L119
[2]   INTERSTELLAR POLYCYCLIC AROMATIC-HYDROCARBONS - THE INFRARED-EMISSION BANDS, THE EXCITATION EMISSION MECHANISM, AND THE ASTROPHYSICAL IMPLICATIONS [J].
ALLAMANDOLA, LJ ;
TIELENS, AGGM ;
BARKER, JR .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1989, 71 (04) :733-775
[3]   POLYCYCLIC AROMATIC-HYDROCARBONS AND THE UNIDENTIFIED INFRARED-EMISSION BANDS - AUTO EXHAUST ALONG THE MILKY-WAY [J].
ALLAMANDOLA, LJ ;
TIELENS, AGGM ;
BARKER, JR .
ASTROPHYSICAL JOURNAL, 1985, 290 (01) :L25-L28
[4]   Theoretical modeling of infrared emission from neutral and charged polycyclic aromatic hydrocarbons. I. [J].
Bakes, ELO ;
Tielens, AGGM ;
Bauschlicher, CW .
ASTROPHYSICAL JOURNAL, 2001, 556 (01) :501-514
[5]   ANHARMONICITY AND THE INTERSTELLAR POLYCYCLIC AROMATIC HYDROCARBON INFRARED-EMISSION SPECTRUM [J].
BARKER, JR ;
ALLAMANDOLA, LJ ;
TIELENS, AGGM .
ASTROPHYSICAL JOURNAL, 1987, 315 (01) :L61-L65
[6]   The infrared spectra of polycyclic aromatic hydrocarbons containing a five-membered ring: symmetry breaking and the B3LYP functional [J].
Bauschlicher, CW ;
Hudgins, DM ;
Allamandola, LJ .
THEORETICAL CHEMISTRY ACCOUNTS, 1999, 103 (02) :154-162
[7]   UV irradiation of polycyclic aromatic hydrocarbons in ices: Production of alcohols, quinones, and ethers [J].
Bernstein, MP ;
Sandford, SA ;
Allamandola, LJ ;
Gillette, JS ;
Clemett, SJ ;
Zare, RN .
SCIENCE, 1999, 283 (5405) :1135-1138
[8]   THE INFRARED-EMISSION BANDS .2. A SPATIAL AND SPECTRAL STUDY OF THE ORION BAR [J].
BREGMAN, JD ;
ALLAMANDOLA, LJ ;
TIELENS, AGGM ;
GEBALLE, TR ;
WITTEBORN, FC .
ASTROPHYSICAL JOURNAL, 1989, 344 (02) :791-798
[9]   Infrared Space Observatory's discovery of C4H2, C6H2, and benzene in CRL 618 [J].
Cernicharo, J ;
Heras, AM ;
Tielens, AGGM ;
Pardo, JR ;
Herpin, F ;
Guélin, M ;
Waters, LBFM .
ASTROPHYSICAL JOURNAL, 2001, 546 (02) :L123-L126
[10]   Simulated infrared emission spectra of highly excited polyatomic molecules: A detailed model of the PAH-UIR hypothesis [J].
Cook, DJ ;
Saykally, RJ .
ASTROPHYSICAL JOURNAL, 1998, 493 (02) :793-802