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首页> 外文期刊>The Astrophysical journal >Synthesis of CO and CO2 Molecules by UV Irradiation of Water Ice-covered Hydrogenated Carbon Grains
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Synthesis of CO and CO2 Molecules by UV Irradiation of Water Ice-covered Hydrogenated Carbon Grains

机译:水冰覆盖的氢化碳粒的紫外线辐照合成CO和CO2分子

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摘要

We present the results of UV irradiation with Lyα photons of carbon grains with a water ice cap at 11 K. Formation of CO and CO2 molecules takes place during irradiation. An estimation of the formation cross section of these molecules by Lyα photons has been obtained from the intensity increase of their infrared stretching bands as a function of the photon fluence. The fraction of carbon in the grains converted to CO and CO2 by UV photons is 0.06 and 0.05, respectively. The spectral profile of the CO stretching feature and that of the CO2 bending mode indicate a polar environment for these molecules. On the basis of the present laboratory results and those obtained in previous work on ion irradiation of similar samples, it has been possible to estimate the contribution of polar CO and CO2 produced on carbon grains by energetic processing to the observed column densities of these molecules for dense clouds whose visual extinction is known. A significant amount of polar CO and CO2 is produced through the mechanism we have studied. Furthermore, we have found that the laboratory profile of the bending band of CO2 produced on carbon grains is compatible with that observed toward the field star Elias 16.
机译:我们介绍了在11 K下用水冰帽用碳粒的Lyα光子进行UV照射的结果。CO和CO2分子的形成在照射过程中发生。从它们的红外拉伸带的强度增加作为光子注量的函数,可以得出由Lyα光子形成的这些分子的横截面的估算值。通过UV光子转换为CO和CO2的晶粒中碳的比例分别为0.06和0.05。 CO拉伸特征的光谱图和CO2弯曲模式的光谱图表明了这些分子的极性环境。根据目前的实验室结果以及先前在类似样品的离子辐照工作中获得的结果,有可能估算出通过能量处理在碳颗粒上产生的极性CO和CO2对这些分子的观察柱密度的贡献。已知其灭绝的密云。通过我们研究的机理,产生了大量的极性CO和CO2。此外,我们已经发现,在碳粒上产生的CO2弯曲带的实验室分布与向野外星Elias 16观测到的弯曲分布是兼容的。

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