Collaborative Research: Dust, Gas, and Star Formation: Synthesizing 20 Years of Radio, Millimeter, and Infrared Surveys

合作研究：尘埃、气体和恒星形成：综合 20 年的无线电、毫米波和红外勘测

• 批准号: 1615728
• 负责人: Karin Sandstrom
• 金额: $ 37.96万
• 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: 2016
• 资助国家: 美国
• 起止时间: 2016-09-01 至 2020-12-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1615728&HistoricalAwards=false
• 关键词: Collaborative; Research; Dust; Gas; Star

Galaxies grow by converting interstellar gas into new generations of stars. A main step in that process is the conversion of low-density, atomic gas into cold, dense, star-forming clouds. Interstellar dust controls this process by shielding gas from destructive ultraviolet radiation and promoting chemical reactions. The abundance of both dust and cold gas depend on local environment in a galaxy, but the nature of this dependence is still debated at a very basic level. This project will test competing hypotheses for what sets the amount of dust and cold gas in galaxies by mapping dust, neutral interstellar gas (diffuse atomic gas and cold, dense molecular gas), and local conditions in a sample of nearby galaxies ten times larger than those used in previous studies. The investigators will use these observations database to answer two questions about gas and star formation in galaxies. The first question is what sets the amount of cold, star-forming gas? The second question is what determines the abundance of dust? These two intertwined questions are critical to understand how galaxies grow and change over time.The investigators will assemble the next generation database of dust and gas distributions in galaxies. To do this, they will combine new and archival observations of atomic hydrogen (HI) from the NSF-funded Very Large Array with Herschel spacecraft measurements of the distribution and properties of interstellar dust. They will increase, by an order of magnitude, the sample of galaxies with such observations. An order of magnitude increase in the set of galaxies studied in this way will advance the field into a new regime of statistical hypothesis testing, a potentially transformative step in understanding the physics of gas in galaxies.The observing database will be shared on the internet with other astronomers and also the public. The investigators will build on the Zooniverse project to share their observations with the public. Zooniverse is an internet tool that allows the public to view and classify scientific observations. With this tool, the public can both appreciate the observations and aid in the research. The investigators plan to create 'the HI Holes Project', in which volunteer citizen scientists will identify giant holes in the gaseous interstellar medium of real and simulated galaxies.

星系团通过将星际气体转化为新一代的恒星而成长。这个过程的一个主要步骤是将低密度的原子气体转化为寒冷、致密的恒星形成云。星际尘埃通过保护气体免受破坏性紫外线辐射和促进化学反应来控制这一过程。尘埃和冷气体的丰度取决于星系中的局部环境，但这种依赖性的性质仍然在非常基本的水平上存在争议。该项目将通过绘制尘埃、中性星际气体（弥漫的原子气体和冷而致密的分子气体）以及比以前研究中使用的样本大十倍的附近星系的局部条件，来测试关于星系中尘埃和冷气体数量的相互竞争的假设。研究人员将利用这些观测数据库来回答两个关于星系中气体和星星形成的问题。 第一个问题是，是什么决定了寒冷的恒星形成气体的数量？ 第二个问题是什么决定了尘埃的丰度？这两个交织在一起的问题对于理解星系如何随着时间的推移而成长和变化至关重要。研究人员将组装下一代星系中尘埃和气体分布的数据库。为了做到这一点，他们将联合收割机结合新的和档案观测原子氢（HI）从国家科学基金会资助的甚大阵列与赫歇尔航天器测量的分布和性质的星际尘埃。 他们将增加一个数量级，星系的样本与这样的观测。 以这种方式研究的星系数量级的增加将推动该领域进入统计假设检验的新领域，这是理解星系中气体物理学的潜在变革性步骤。观测数据库将在互联网上与其他天文学家和公众共享。 研究人员将在Zooniverse项目的基础上与公众分享他们的观察结果。 Zooniverse是一个互联网工具，允许公众查看和分类科学观察。 有了这个工具，公众既可以欣赏观察结果，也可以帮助研究。研究人员计划创建“HI洞项目”，其中志愿公民科学家将在真实的和模拟星系的气态星际介质中识别巨大的洞。