ABSOLUTE PHOTODETACHMENT CROSS-SECTION MEASUREMENTS FOR HYDROCARBON CHAIN ANIONS

被引:53
|
作者
Best, T. [1 ,2 ]
Otto, R. [1 ,2 ]
Trippel, S. [2 ]
Hlavenka, P. [2 ]
von Zastrow, A. [2 ]
Eisenbach, S. [2 ]
Jezouin, S. [2 ]
Wester, R. [1 ,2 ]
Vigren, E. [3 ]
Hamberg, M. [3 ]
Geppert, W. D. [3 ]
机构
[1] Univ Innsbruck, Inst Ionenphys & Angew Phys, A-6020 Innsbruck, Austria
[2] Univ Freiburg, Inst Phys, D-79104 Freiburg, Germany
[3] Stockholm Univ, Div Mol Phys, S-10691 Stockholm, Sweden
来源
ASTROPHYSICAL JOURNAL | 2011年 / 742卷 / 02期
关键词
astrochemistry; ISM: molecules; molecular data; molecular processes; MASS PROTOSTAR IRAS-04368+2557; DIFFUSE INTERSTELLAR BANDS; NEGATIVE-IONS; ASTRONOMICAL IDENTIFICATION; L1527; C6H; C4H; C8H; IRC+10216; THRESHOLD;
D O I
10.1088/0004-637X/742/2/63
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Absolute photodetachment cross sections have been measured for the hydrocarbon chain anions CnH-, n = 2, 4, and 6, which are relevant for an understanding of molecular clouds in the interstellar medium. Data have been obtained for different photon energies within approximately 1 eV of the detachment threshold. With our recently developed method we have achieved a precision of better than 25% on these absolute cross sections. The experiments have been carried out by means of photodetachment tomography of the mass-selected molecular anions in a multipole radio-frequency ion trap. The measured absolute cross sections are in accordance with the empirical scaling law of Millar et al. and have allowed us to determine its free parameters. These results are important for predicting the photostability and thus the abundance of carbon chain anions in planetary atmospheres, in circumstellar envelopes, and in photon-dominated regions of interstellar molecular clouds.
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页数:6
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