Modelling spectra of pre-main sequence and magnetic sequence stars

前主序星和磁序星的光谱建模

• 批准号: 6377-2010
• 负责人: Landstreet, John
• 金额: $ 2.33万
• 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: 2013
• 资助国家: 加拿大
• 起止时间: 2013-01-01 至 2014-12-31
• 项目状态: 已结题
• 来源: https://www.nserc-crsng.gc.ca/ase-oro/Details-Detailles_eng.asp?id=520913
• 关键词: Modelling; spectra; pre; main; sequence

Astronomers now understand the broad outlines of how stars form, how they change through their lives, and what happens to them when they run out of fuel and collapse or explode. However, important steps in this life story are still poorly or hardly understood.

天文学家现在了解了恒星如何形成的大致轮廓，它们在生命中如何变化，以及当它们耗尽燃料并崩溃或爆炸时会发生什么。然而，这个生命故事中的重要步骤仍然很少或几乎不被理解。