候选星际芳香分子的红外辐射光谱
D J Cook1, S Schlemmer, N Balucani
1Department of Chemistry, University of California, Berkeley 94720-1460, USA.
多环芳 (PAH) 是恒星形成的关键. 实验室光谱显示中性PAH对星际红外波段的贡献很小,但它们的充电形式和更大的PAH仍然是可能的来源.
科学领域:
- 天体化学是天体化学.
- 天体物理学 天体物理学
- 频谱学是一种光谱学.
背景情况:
- 星际尘埃促进分子的形成,这对于恒星的诞生至关重要.
- 多环芳 (PAH) 是太空中大量存在的碳化合物,可能形成尘埃并解释红外辐射.
- 了解PAH排放对于解释星际光谱至关重要.
研究的目的:
- 在模拟的星际条件下研究各种PAH的辐射光谱.
- 为了确定中性和电离型PAHs对未确定的红外辐射波段的贡献.
- 为了确定观测到的星际红外特征的潜在来源.
主要方法:
- 获取代表PAHs的实验室排放光谱.
- 模拟星际介质条件用于光谱测量.
- 分析整个未识别红外波段的光谱.
主要成果:
- 小到中等尺寸的中性PAH仅对未识别的红外波段做出了微小的贡献.
- 排放光谱表明,电离型PAHs是更重要的贡献者.
- 较大的PAH及其离子也是观察到的排放的可行候选物.
结论:
- 中性PAH不太可能是未确定的红外辐射波段的主要来源.
- 电离PAH和更大的PAH分子仍然是解释这些星际光谱特征的强有力的候选者.
- 需要进一步研究电离和大PAH的光谱特性.
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