Resolving the Structure of Photodissociation Regions at Low Metallicity

解析低金属丰度下光解离区域的结构

• 批准号: 2308274
• 负责人: Karin Sandstrom
• 金额: $ 40.25万
• 依托单位: University of California-San Diego
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2023
• 资助国家: 美国
• 起止时间: 2023-09-01 至 2026-08-31
• 项目状态: 未结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2308274&HistoricalAwards=false
• 关键词: Resolving; Structure; Photodissociation; Regions; Low

Photodissociation regions (PDRs) --- interstellar gas whose properties are determined by far-ultraviolet radiation --- govern the formation of cold, dense, molecular gas where star formation can occur. This research project will use high quality observations from the Atacama Large Millimeter/submillimeter Array (ALMA) to resolve and characterize the different layers of gas within PDRs in the Small Magellanic Cloud (SMC). The processes within PDRs are sensitive to the abundance of heavy elements, and the SMC is poor in heavy elements relative to the Milky Way, so the results from this project will help shed light on how physical conditions within PDRs depend on the “metallicity” of the gas. The project will train a graduate student in methods of advanced astronomical research, and it will develop a program to facilitate the participation of incoming community college transfer students in undergraduate research. The investigators have obtained new ALMA observations that resolve the structure of a PDR in the low metallicity environment of the SMC. They will undertake three efforts to characterize the observed PDR. First, they will measure the temperature of the gas using the rotational emission lines of carbon monoxide (CO) and the fine structure lines of neutral carbon (C), comparing the measurements to PDR models. Next, they will compare the location of the atomic-to-molecular hydrogen (H/H2) transition to the C+/C/CO transition to study the nature of “CO-dark H2 gas” --- PDR layers where hydrogen is molecular (H2) while carbon is either ionized (C+) or neutral. Finally, they will use the high velocity resolution possible with ALMA to study the dynamics and turbulence of gas in the PDR.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

光离解区（PDR）---星际气体，其性质由远紫外线辐射决定---控制着冷的、致密的分子气体的形成，在那里星星可以形成。 该研究项目将使用来自阿塔卡马大型毫米/亚毫米阵列（阿尔马）的高质量观测来解析和表征小麦哲伦云（SMC）中PDR内的不同气体层。 PDR内的过程对重元素的丰度很敏感，而SMC相对于银河系来说重元素很少，因此该项目的结果将有助于阐明PDR内的物理条件如何取决于气体的“金属性”。 该项目将对一名研究生进行高级天文学研究方法方面的培训，并将制定一项方案，以促进即将入学的社区学院转学生参与本科生研究。研究人员已经获得了新的阿尔马观测结果，解决了SMC低金属含量环境中PDR的结构。他们将作出三项努力，以确定所观察到的公共民主报告的特点。 首先，他们将使用一氧化碳（CO）的旋转发射谱线和中性碳（C）的精细结构谱线测量气体的温度，并将测量结果与PDR模型进行比较。接下来，他们将比较原子到分子的氢（H/H2）跃迁与C+/C/CO跃迁的位置，以研究“CO-暗H2气体”的性质-- PDR层，其中氢是分子（H2），而碳是离子化的（C+）或中性的。 最后，他们将利用阿尔马可能的高速度分辨率来研究PDR中气体的动力学和湍流。该奖项反映了NSF的法定使命，并通过使用基金会的知识价值和更广泛的影响审查标准进行评估，被认为值得支持。