在星际介质中检测芳香分子 (c-C6H5CN)
Brett A McGuire1,2, Andrew M Burkhardt3, Sergei Kalenskii4
1National Radio Astronomy Observatory, Charlottesville, VA 22903, USA.
概括
天文学家在星际环境中发现了一种简单的芳香分子, 这一发现可能将含的简单芳与未确定的红外波段的载体联系起来.
科学领域:
- 天体化学
- 星际介质的组成
- 芳香分子的识别
背景情况:
- 假设多环芳 (PAH) 和它们含的类似物 (异环) 在太空中大量存在.
- 这些分子被怀疑是各种天文来源中观察到的未识别红外 (UIR) 发射波段的载体.
- 在星际介质中直接识别特定的芳香分子是具有挑战性的.
研究的目的:
- 在星际介质中识别特定的含芳香分子.
- 研究简单的芳香分子作为更大的PAH的前体的潜在作用.
- 在观测到的星际分子和UIR带载体之间建立化学联系.
主要方法:
- 在排放中观察酸 (c-C6H5CN) 的超精度过渡.
- 使用无线电天文学技术检测来自分子云TMC-1的光谱线.
主要成果:
- 在星际介质中首次确切地发现酸 (c-C6H5CN).
- 在TMC-1分子云中进行了观测,目标是特定的排放线.
- 通过其独特的高精度分辨率的光谱过渡来识别尼.
结论:
- 在星际空间发现了一种含的简单芳香分子,
- 这一发现提供了基本芳香成分的观测证据.
- 尼可以作为形成较大的多环芳的前体分子,这可能解释了UIR波段.
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