Theoretical Studies in Star Formation

恒星形成的理论研究

• 批准号: 0606831
• 负责人: Christopher McKee
• 金额: $ 42.1万
• 依托单位: University of California-Berkeley
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2006
• 资助国家: 美国
• 起止时间: 2006-07-01 至 2010-06-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0606831&HistoricalAwards=false
• 关键词: Theoretical; Studies; Star; Formation

AST-0606831INSTITUTION: University of California, BerkeleyPI: Christopher McKeeCo-PI: Richard KleinTITLE: Theoretical Studies in Star FormationABSTRACTDr. Christopher McKee and Dr. Richard Klein, at the University of California, Berkeley, will study a wide range of fundamental issues relating to the star formation process. Among the projects they will undertake will be modeling of the neutral and molecular components of the interstellar medium in the Milky Way and in M31, with a comparison of the model predictions to observations. Additionally they will work toward development of a model that predicts star formation rates and molecular fractions of galaxies for use in cosmological simulations. Dr. McKee and Dr. Klein will also work toward simulating the evolution of giant molecular clouds and the generation of turbulence, modeling the formation of massive clusters, adding ambipolar diffusion to simulations of the collapse of magnetized cores, and modeling the evolution of HII regions.Dr. McKee and Dr. Klein will also train graduate students, with a goal of adding to the diversity of the scientific work force.

美国加州大学伯克利分校出版：Christopher McKeeco-Pi：Richard KleinTitle：恒星形成理论研究摘要加州大学伯克利分校的克里斯托弗·麦基和理查德·克莱因博士将研究与恒星形成过程相关的一系列基本问题。在他们将开展的项目中，将对银河系和M31星际介质的中性和分子成分进行建模，并将模型预测与观测进行比较。此外，他们还将致力于开发一种模型，预测恒星形成速度和星系的分子分数，用于宇宙学模拟。McKee博士和Klein博士还将致力于模拟巨型分子云的演化和湍流的产生，对大质量星系团的形成进行建模，将双极扩散添加到对磁化核心坍塌的模拟中，并对HII区域的演变进行建模。McKee和Klein博士还将培训研究生，目标是增加科学工作者的多样性。