未识别的星际红外波段:PAHs作为载体?
S Schlemmer1, D J Cook, J A Harrison
1Department of Chemistry, University of California, Berkeley 94720-1460, USA.
概括
实验室内红外光谱的甲和烯不与天文观测相匹配. 这表明,小的多环芳碳化合物并不负责太空中未确定的红外辐射波段.
科学领域:
- 天体化学是天体化学.
- 频谱学是一种光谱学方法.
背景情况:
- 天文物体表现出未识别的红外辐射波段.
- 多环芳 (PAHs) 是这些频段的潜在载体.
- 纳夫他林和烯是代表性的小,未被替代的PAHs.
研究的目的:
- 用于测量气相甲烯和烯的红外辐射光谱.
- 将实验室光谱与未识别红外辐射波段的天文观测进行比较.
- 为了确定小,未被替代的PAH是否可以解释天文观测.
主要方法:
- 测量了气相甲烯和烯的红外辐射光谱.
- 测量是在3至7.5微米范围内进行的.
- 采用紫外线激光溶解激发和单光子计数红外光谱学.
主要成果:
- 在实验室光谱和天文数据之间观察到显著的差异.
- 波长和光谱特征的相对强度不匹配.
- 实验室的甲和二烯的辐射光谱并没有复制观察到的天文频段.
结论:
- 小型,中性,未被替代的多环芳是未识别红外辐射波段的不太可能载体.
- 天文学物体中未识别的红外辐射波段的起源仍然是未知的.
- 需要进一步的研究来确定负责这些光谱特征的分子.
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