Towards a global understanding of high mass star formation

全面了解高质量恒星的形成

• 批准号: 249680-2011
• 负责人: Plume, René
• 金额: $ 2.04万
• 依托单位: University of Calgary
• 依托单位国家: 加拿大
• 项目类别: Discovery Grants Program - Individual
• 财政年份: 2012
• 资助国家: 加拿大
• 起止时间: 2012-01-01 至 2013-12-31
• 项目状态: 已结题
• 来源: https://www.nserc-crsng.gc.ca/ase-oro/Details-Detailles_eng.asp?id=507428
• 关键词: Towards; global; understanding; mass; star

Over the past 20 years there have been significant advances in the field of star formation. We have determined that all stars are born deeply embedded and emerge over time as the surrounding material is either accreted or dispersed. We have discovered InfraRed Dark Clouds which are cold, dense clouds of gas and dust seen in silhouette against the bright mid-infrared background produced by the Galactic Plane and learned that they are likely the progenitors of young stars, including stars more massive than the Sun. We have also learned that the chemical composition of the gas in a star forming region can have an effect on its physical evolution. A large part of our progress in the field of star formation has focused solely on the formation of low-mass stars, predominantly because these objects form isolated from other nearby stars, reducing confusion. However, it has now been recognized that most stars, and especially stars more massive than the Sun, do not form in an isolated fashion. Instead, over approximately 90% of all stars form in clusters, in regions which are also forming massive stars. Similar progress in our understanding of the formation of massive stars has been hampered by several factors: a) The greater distances of the Giant Molecular Clouds that are the birth sites of massive stars makes studies of individual objects difficult. b) Contraction timescales for massive stars are much shorter meaning that examples of the earliest phases are rare. c) The very nature of clustered star formation increases the chances for confusion. As a result, even though massive stars are key drivers of energy production and heavy element abundance in the Galaxy, their formation mechanism is unclear. In this proposal, funding is requested to tackle some of the most pressing issues in the field of massive star formation. What are the properties (physical & velocity structure, density, temperature, chemical abundances, etc.) of massive star forming regions? What makes them different from regions forming low mass stars? How do the clouds that give birth to massive stars form in the first place?

在过去的20年里，在星星的形成领域取得了重大进展。我们已经确定，所有的恒星出生时都深深地嵌入其中，随着时间的推移，随着周围物质的吸积或分散而出现。 我们已经发现了红色的暗云，这是一种冷的，致密的气体和尘埃云，在银河系平面产生的明亮的中红外背景下可以看到轮廓，并了解到它们可能是年轻恒星的祖先，包括比太阳更大的恒星。 我们还了解到，星星形成区气体的化学成分会对其物理演化产生影响。 我们在星星形成领域的很大一部分进展仅仅集中在低质量恒星的形成上，主要是因为这些物体与附近的其他恒星隔离，减少了混乱。然而，现在人们已经认识到，大多数恒星，特别是质量比太阳大的恒星，并不是孤立形成的。相反，超过90%的恒星形成于星团中，这些区域也形成了大质量恒星。在我们对大质量恒星形成的理解中，类似的进展受到以下几个因素的阻碍：a）大质量恒星诞生地巨分子云的距离更远，使得对单个物体的研究变得困难。B）大质量恒星的收缩时间尺度要短得多，这意味着最早阶段的例子很罕见。c）聚集星星形成的本质增加了混淆的机会。因此，尽管大质量恒星是银河系能量产生和重元素丰度的关键驱动力，但它们的形成机制尚不清楚。在这项提案中，要求提供资金，以解决大质量星星形成领域中一些最紧迫的问题。 有什么性质（物理和速度结构，密度，温度，化学丰度等）大质量星星形成区的位置 是什么使它们不同于形成低质量恒星的区域？产生大质量恒星的云首先是如何形成的？