Astrophysical Processes in the ISM

ISM 中的天体物理过程

• 批准号: RGPIN-2016-04460
• 负责人: Houde, Martin
• 金额: $ 2.91万
• 依托单位: University of Western Ontario
• 依托单位国家: 加拿大
• 项目类别: Discovery Grants Program - Individual
• 财政年份: 2020
• 资助国家: 加拿大
• 起止时间: 2020-01-01 至 2021-12-31
• 项目状态: 已结题
• 来源: https://www.nserc-crsng.gc.ca/ase-oro/Details-Detailles_eng.asp?id=709322
• 关键词: Astrophysical; Processes; ISM

How do galaxies form? How do planets form? Where do we come from? Are we really made of stardust? Although these questions deal with subjects of vastly different scales (i.e., the galactic, planetary, human, and microscopic scales), they are all linked together through the different astrophysical processes that rule and organize the cosmos. The origin of the stars themselves, however, is arguably the single most important topic that underlies these and other fundamental astrophysical questions. As stars form they acquire the characteristics that will determine how they will live their life, affect their galactic neighbourhood, and ultimately die. The problem of understanding the different processes and phases of star formation is central to obtaining a better and bigger picture of the working of the Galaxy and the Universe as a whole. This research program proposes to attack problems, including star formation, by studying the astrophysical processes that take place in molecular clouds and other regions within our Galaxy. Molecular clouds are aggregates of dust and gas that serve as the birthplace of stars, while also constituting one of the main components of our Galaxy. Because of their fundamental position in the time line that spans the life of stars, a study of molecular clouds, and the processes they harbour, is also a study of star formation. The program will concentrate on two of the agents and phenomena that are known to inhabit these structures: the interstellar magnetic field and gas turbulence, as well as fundamental small-scale interactions between atoms, molecules, and radiation. It is expected within only a few years to provide a wealth of new data that will significantly improve our understanding of many aspects of the interstellar medium and the star formation process.

星系是如何形成的？行星是如何形成的？我们从哪里来？我们真的是由星尘组成的吗？尽管这些问题涉及的主题规模截然不同（即，星系、行星、人类和微观尺度），它们都通过不同的天体物理过程联系在一起，统治和组织宇宙。 然而，恒星本身的起源可以说是构成这些和其他基本天体物理学问题基础的唯一最重要的主题。随着恒星的形成，它们获得的特征将决定它们将如何生活，影响它们的银河系邻居，并最终死亡。理解星星形成的不同过程和阶段的问题，对于更好地了解银河系和整个宇宙的运行情况至关重要。 该研究计划提出通过研究分子云和银河系其他区域中发生的天体物理过程来解决包括星星形成在内的问题。分子云是尘埃和气体的聚集体，是恒星的诞生地，同时也是银河系的主要组成部分之一。由于分子云在贯穿恒星生命的时间线上的基本位置，对分子云及其所包含的过程的研究也是对星星形成的研究。该计划将集中在已知存在于这些结构中的两种代理和现象：星际磁场和气体湍流，以及原子，分子和辐射之间的基本小尺度相互作用。预计在短短几年内，它将提供丰富的新数据，将大大提高我们对星际介质和星星形成过程的许多方面的理解。