THE NASA AMES POLYCYCLIC AROMATIC HYDROCARBON INFRARED SPECTROSCOPIC DATABASE: THE COMPUTED SPECTRA

被引：169

作者：

Bauschlicher, C. W., Jr. ^{[1
]}

Boersma, C. ^{[1
,2
]}

Ricca, A. ^{[1
,3
]}

Mattioda, A. L. ^{[1
,3
]}

Cami, J. ^{[1
,3
,4
]}

Peeters, E. ^{[1
,3
,4
]}

de Armas, F. Sanchez ^{[3
]}

Saborido, G. Puerta ^{[3
]}

Hudgins, D. M. ^{[5
]}

Allamandola, L. J. ^{[1
]}

机构：

[1] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA

[2] Univ Groningen, Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands

[3] SETI Inst, Mountain View, CA 94043 USA

[4] Univ Western Ontario, Dept Phys & Astron, PAB 213, London, ON N6A 3K7, Canada

[5] NASA Headquarters, Washington, DC 20546 USA

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2010年 / 189卷 / 02期

关键词：

astrochemistry; ISM: lines and bands; methods: laboratory; methods: numerical; molecular data; techniques: spectroscopic; PHASE PAH MOLECULES; INTERSTELLAR DUST; EMISSION SPECTRA; BENDING MODES; BANDS; GAS; APPROXIMATION; NAPHTHALENE; ABSORPTION; PROFILES;

D O I：

10.1088/0067-0049/189/2/341

中图分类号：

P1 [天文学];

学科分类号：

070403 [天体物理学];

摘要：

The astronomical emission features, formerly known as the unidentified infrared bands, are now commonly ascribed to polycyclic aromatic hydrocarbons (PAHs). The laboratory experiments and computational modeling done at the NASA Ames Research Center to create a collection of PAH IR spectra relevant to test and refine the PAH hypothesis have been assembled into a spectroscopic database. This database now contains over 800 PAH spectra spanning 2-2000 mu m (5000-5 cm(-1)). These data are now available on the World Wide Web at www.astrochem.org/pahdb. This paper presents an overview of the computational spectra in the database and the tools developed to analyze and interpret astronomical spectra using the database. A description of the online and offline user tools available on the Web site is also presented.

引用

页码：341 / 351

页数：11

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