Deuterium chemistry of dense gas in the vicinity of low-mass and massive star-forming regions
Deuterium chemistry of dense gas in the vicinity of low-mass and massive star-forming regions
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低质量和大质量恒星形成区域附近致密气体的氘化学
DOI：
10.1093/mnras/stu1141
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发表时间：
2014
影响因子：
4.8
通讯作者：
Awad Z
中科院分区：
文献类型：
--
作者：
Awad Z
氘与氢原子的标准星际比（D/H）为1.5 × 10−5。然而，氘分馏实际上被发现在不同程度上增强，在冷的暗核心，大质量恒星形成区域周围的热核心，不冷的核心，以及低质量恒星形成区域周围的温暖核心（以下称为热corino）。在本文中，我们调查的整体差异，氘化学之间的热核和热corino。我们用气体颗粒化学模型模拟了低质量和大质量恒星形成区周围致密气体的化学性质。我们研究了不同的核心密度、气体物质对尘埃颗粒的消耗效率、坍缩模式和原恒星的最终质量对恒星形成区化学演化的影响。我们发现，氘化学是，在一般情况下，最敏感的变化的耗尽效率的粮食表面上，与观察一致。此外，结果表明，在热的核心比在热corino的化学是更敏感的坍缩核心的最终密度的变化。最后，我们发现，氘硫轴承物种在致密气体周围的热核心和corinos的比例可能是很好的演化指标，以类似的方式作为他们的非氘同行。
The standard interstellar ratio of deuterium to hydrogen (D/H) atoms is ∼1.5 × 10−5. However, the deuterium fractionation is in fact found to be enhanced, to different degrees, in cold, dark cores, hot cores around massive star-forming regions, lukewarm cores, and warm cores (hereafter hot corinos) around low-mass star-forming regions. In this paper, we investigate the overall differences in the deuterium chemistry between hot cores and hot corinos. We have modelled the chemistry of dense gas around low-mass and massive star-forming regions using a gas-grain chemical model. We investigate the influence of varying the core density, the depletion efficiency of gaseous species on to dust grains, the collapse mode and the final mass of the protostar on the chemical evolution of star-forming regions. We find that the deuterium chemistry is, in general, most sensitive to variations of the depletion efficiency on to grain surfaces, in agreement with observations. In addition, the results showed that the chemistry is more sensitive to changes in the final density of the collapsing core in hot cores than in hot corinos. Finally, we find that ratios of deuterated sulphur bearing species in dense gas around hot cores and corinos may be good evolutionary indicators in a similar way as their non-deuterated counterparts.