在星际介质中检测出一个分支基分子:异烯化物
Arnaud Belloche1, Robin T Garrod2, Holger S P Müller3
1Max-Planck-Institut für Radioastronomie (MPIfR), Auf dem Hügel 69, 53121 Bonn, Germany. belloche@mpifr-bonn.mpg.de.
概括
天文学家在星际空间中发现了异烯化物,一种分支的有机分子. 这一发现表明,对氨基酸至关重要的分支分子在宇宙中很常见.
科学领域:
- 天体化学是天体化学.
- 星际介质的组成 星际介质的组成
- 有机分子的形成
背景情况:
- 在星际介质 (ISM) 中发现的最大的非循环分子是具有直链碳骨干的有机化合物.
- 之前在ISM中的检测主要集中在线性有机分子上.
研究的目的:
- 报告第一个分支基分子的星际检测,异烯化物 (i-C3H7CN).
- 调查这一检测对ISM中分支碳链分子丰富性的影响.
- 探索ISM中线性和分支的有机分子的形成途径.
主要方法:
- 在ISM中进行分子检测的天文学观测.
- 天体化学建模以模拟分子形成路径.
- 分支异烯化物及其直链异构体之间的丰度比较.
主要成果:
- 在星际介质中检测出异烯化物 (i-C3H7CN).
- 发现异烯酸的丰富度是其直链同位素的0.4倍.
- 天体化学模型表明,这两种异构体都通过激素添加,通过不同的途径在尘埃粒冰层上形成.
结论:
- 检测到异烯化物表明,分支碳链分子可能在ISM中普遍丰富.
- 异烯酸的形成需要对非终端碳添加功能组,这表明复杂分子合成的途径.
- 这一发现支持ISM中氨基酸的潜在存在,这些氨基酸具有类似的分支侧链结构.
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