在星际云中通过与C2H2,HS和原子H的冰反应形成S轴承复杂有机分子
Julia C Santos1, Joan Enrique-Romero2, Thanja Lamberts2,3
1Laboratory for Astrophysics, Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands.
概括
这项研究表明,硫化合物如何在冰冷的星际环境中形成. 实验室实验表明,SH基与乙反应,产生各种含硫分子,包括乙醇.
科学领域:
- 天体化学是天体化学.
- 星际化学 星际化学
- 实验室天体物理学
背景情况:
- 星际硫的化学网络由于丰富度差异,人们对其了解甚少.
- 最近对含硫有机分子的检测突显了形成途径研究的必要性.
研究的目的:
- 在10K时研究乙和SH基的固态化学.
- 确定在星际冰层条件下形成的硫化产品.
- 在星际硫化学中阐明反应路径.
主要方法:
- 实验室实验模拟星际冰罩.
- 乙 (C2H2) 的固态反应与SH基在10K.
- 使用反射吸收红外光谱学和四极质谱学进行分析,采用温度编程的脱吸.
主要成果:
- 确认的SH激素启动星际硫化学.
- 确定了六种硫化产品:乙醇 (CH3CH2SH),乙烯 (CH2CHSH),滴醇 (HSCH2CH2SH),二硫化 (H2S2),以及暂时的乙 (CH3CHS) 和乙烯 (CH2CS).
- 乙醇是形成的主要有机硫分子,其产量随着的丰富而增加.
结论:
- 在星际冰中启动硫化学过程中,SH激素至关重要.
- 拟议的化学网络解释了关键的含硫分子的形成.
- 乙醇作为该网络中硫的重要消化器,影响了其他不和产品的丰度.
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