Globular Clusters: Diagnostic Indicators of Halo Structure, Galaxy Formation and Interaction Histories

球状星团：晕结构、星系形成和相互作用历史的诊断指标

• 批准号: 8545-2013
• 负责人: Hanes, David
• 金额: $ 1.53万
• 依托单位: Queen's University
• 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=521146
• 关键词: Globular; Clusters; Diagnostic; Indicators; Halo

The observable universe is bespangled with luminous galaxies, many of them much larger than our own majestic Milky Way, the grand spiral within which the Sun is located. The galaxies themselves may contain literally trillions of Sun-like stars and take on a variety of forms. They are not arranged at random in space, but instead are clustered together or distributed in vast walls and enormous streamers on almost unimaginably large spatial scales. Yet although we can discern and map out the physical distributions of these individual cities of stars, the study of their origin and formation history remains an incompletely resolved question in the science of cosmology. How did they come to be? Fortunately, the galaxies themselves contain important fossil records of their youthful stages -- namely, the rich, supremely beautiful globular star clusters that move in stately orbits around the galaxies, held in a gravitational embrace. Our Milky Way has more than one hundred such star clusters; in other galaxies, there may be tens of thousands. Using the largest telescopes, we can metaphorically 'dissect' the globulars, even in galaxies tens of millions of light years away, spreading the combined light emitted by their constituent stars into a colourful spectrum. We then analyse features in the spectrum to determine the age, chemical composition, and state of orbital motion of each cluster around its parent galaxy. This knowledge takes on enormous significance when coupled with the fact that the globular clusters are the oldest known stellar objects in the visible universe. Their nature and dynamics, therefore, tell us about the turbulent formative processes that marked a galaxy's birth, more than ten billion years ago. Moreover, a complex mix and range of these attributes among the many hundreds or thousands of clusters will also indicate whether a galaxy has suffered a subsequent vigorous interaction -- or even a catastrophic merger -- with a sister galaxy. Interestingly, predictions of the future behaviour of our own Milky Way seem inevitably to yield a merger with the nearby Andromeda spiral galaxy, a mere two million light years away. The globular clusters have the power to tell us how common such events are in galaxy formation histories.

可观测的宇宙中布满了发光的星系，其中许多比我们所在的壮观的银河系要大得多，银河系是太阳所在的大螺旋星系。这些星系本身可能包含数万亿颗类似太阳的恒星，并呈现出各种形式。它们并不是在空间上随机排列的，而是聚集在一起或分布在巨大的墙壁和巨大的彩带中，空间规模几乎难以想象。然而，尽管我们可以辨别和绘制出这些单个恒星城市的物理分布，但它们的起源和形成历史的研究在宇宙学中仍然是一个尚未完全解决的问题。它们是如何形成的？幸运的是，星系本身包含了它们年轻阶段的重要化石记录--也就是丰富、极其美丽的球状星团，它们沿着庄严的轨道围绕星系运动，处于引力的怀抱中。我们的银河系有一百多个这样的星团；在其他星系，可能有数万个。使用最大的望远镜，我们可以比喻地‘解剖’球状星体，即使是在数千万光年之外的星系中，将它们的组成恒星发出的组合光扩散成五颜六色的光谱。然后，我们分析光谱特征，以确定每个星系团围绕其母星系的年龄、化学成分和轨道运动状态。当球状星团是可见宇宙中已知的最古老的恒星物体时，这一知识就具有了巨大的意义。因此，它们的性质和动力学告诉我们100多亿年前标志着一个星系诞生的动荡的形成过程。此外，在成百上千的星系团中，这些属性的复杂混合和范围也将表明一个星系是否经历了随后的激烈相互作用--甚至是灾难性的合并--与姐妹星系。有趣的是，对我们银河系未来行为的预测似乎不可避免地会导致与附近的仙女座螺旋星系合并，后者距离我们只有200万光年。球状星团有能力告诉我们，在星系形成历史上，这样的事件是多么常见。