Comprehensive Study of Atomic & Molecular Gas in Taurus: Evolution of the Interstellar Medium and Star Formation

原子综合研究

• 批准号: 0407019
• 负责人: Paul Goldsmith
• 金额: --
• 依托单位: Cornell University
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2004
• 资助国家: 美国
• 起止时间: 2004-11-01 至 2010-07-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0407019&HistoricalAwards=false
• 关键词: Comprehensive; Study; Atomic; & Molecular

AST 0407019GoldsmithDr. Paul Goldsmith will carry out a major study of the Taurus molecular cloud complex. It will result in the largest images in 12CO and 13CO of a molecular cloud yet obtained. This project will also produce the first fully sampled high angular resolution map of atomic hydrogen in the 100 square degree region. The combination of the atomic and molecular data sets will, in conjunction with existing data on the dust distribution and young stars in Taurus, provide a unique tool for studying key aspects of the life cycle of molecular clouds and star formation.Acquiring the data to address these important questions is only possible due to recent developments in radio astronomical imaging technology. The molecular maps will be obtained using the Five College Radio Astronomy Observatory 13.7m telescope and 32 element Sequoia focal plane array: observing time has already been allocated. The HI data will be obtained using the 305m Arecibo telescope and the 7 element dual polarization ALFA focal plane array system. Prior to the availability of these instruments which provide an order of magnitude increase inmapping speed, it was not realistic to cover the required solid angle with the angular resolution needed to be sensitive to structure over a range of scales exceeding 100:1. The greatly enhanced capability permits this project to address the following key questions. 1. The relationship between the atomic and molecular components of Taurus, including the evolutionary history of the region, will be addressed by comparing the hydrogen emission and absorption line profilesand column densities, and by determining the ages of cloud cores from their residual atomic gas content; 2. The role of turbulence in dark cloud complexes -- both in the atomic/molecular transition and in the formation of new stars -- will be studied by the Dr. Goldsmith and collaborators through identification of critical scales for turbulent support based on Principal Component Analysis; 3. Critical parameters for star formation, including the threshold of column density and/or density, the association between molecular clouds and stars, and the role of large scale processes versus local effects in star formation will be identified; 4. The impact of young stars on molecular clouds and subsequent star formation will be evaluated by carrying out a complete census of molecular outflows, the energy that they have returned to molecular clouds, and their effect on cloud structure. This work will have an impact on a wide range of areas in astrophysics and star formation research, especially (1) numerical simulations of atomic and molecular cloud hydrodynamics including the transition between these two key phases; (2) time dependent astrochemistry based on gas phase reactions and grain surface formation of molecular hydrogen; (3) the overall energetics of molecular clouds including dissipation and regeneration of turbulence. This work will integrate research and teaching. Various portions of the data will be ideal for investigation by undergraduate students. Inasmuch as the formation of solar type stars is of considerable interest to the public, and that this kind of mapping project really does produce images to which people can relate, it is ideally suited for both talks and to be the focus of exhibits being contemplated for local science education facilities.

AST0407019金匠博士保罗·戈德史密斯将对金牛座分子云复合体进行重大研究。这将产生迄今获得的最大的12CO和13CO分子云图像。该项目还将在100平方度区域制作第一张全采样高角度分辨率的氢原子图。原子和分子数据集的结合将结合金牛座尘埃分布和年轻恒星的现有数据，为研究分子云生命周期和恒星形成的关键方面提供独特的工具。只有由于射电天文成像技术的最近发展，才有可能获得这些数据来解决这些重要问题。分子图谱将使用五所大学射电天文台13.7米望远镜和32元红杉焦平面阵列获得：观测时间已经分配。HI数据将使用305m阿雷西博望远镜和7元双偏振阿尔法焦平面阵列系统获得。在这些仪器在测绘速度上提高了一个数量级之前，在超过100：1的比例范围内，用对结构敏感的角度分辨率来覆盖所需的立体角度是不现实的。大大增强的能力使该项目能够解决以下关键问题。1.金牛座的原子和分子组成之间的关系，包括该区域的进化史，将通过比较氢发射和吸收谱线轮廓和柱密度，以及通过根据其残留的原子气体含量确定云核的年龄来解决；2.戈德史密斯博士及其合作者将通过基于主成分分析的湍流支持的临界尺度来研究暗云复合体中湍流的作用--包括在原子/分子跃迁和新星形成中的作用；3.将确定恒星形成的关键参数，包括柱密度和/或密度的阈值，分子云与恒星之间的联系，以及大尺度过程与局部效应在恒星形成中的作用；4.年轻恒星对分子云和后续恒星形成的影响将通过对分子外流、分子云返回的能量及其对云结构的影响进行全面普查来评估。这项工作将对天体物理和恒星形成研究的广泛领域产生影响，特别是(1)原子和分子云流体动力学的数值模拟，包括这两个关键阶段之间的跃迁；(2)基于气相反应和分子氢颗粒表面形成的含时天体化学；(3)分子云的整体能量学，包括湍流的耗散和再生。这项工作将把研究和教学结合起来。这些数据的不同部分将是本科生调查的理想选择。由于太阳类型恒星的形成引起了公众的极大兴趣，而且这种测绘项目确实产生了人们可以联系到的图像，因此它非常适合用于演讲，也是当地科学教育设施正在考虑的展览的焦点。