Star Clusters Near and Far
Star Clusters Near and Far
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DOI：
10.1007/s11214-020-00690-x
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发表时间：
2020-05
影响因子：
10.3
通讯作者：
A. Adamo;Peter Zeidler;Peter Zeidler;J. Kruijssen;M. Chevance;M. Gieles;D. Calzetti;Corinne Charbonnel;Corinne Charbonnel;H. Zinnecker;M. Krause
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文献类型：
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作者：
A. Adamo;Peter Zeidler;Peter Zeidler;J. Kruijssen;M. Chevance;M. Gieles;D. Calzetti;Corinne Charbonnel;Corinne Charbonnel;H. Zinnecker;M. Krause
星星团是恒星反馈的基本单位，也是其宿主星系性质的独特示踪物。在这篇综述中，我们将首先关注它们的成分，即详细了解它们的恒星种群及其周围的电离，温暖，中性和分子气体。然后，我们超越了本星系群，回顾了处于不同进化阶段的星星群，以及在本星系宇宙中可访问的不同银河系环境条件。在高红移时，星团形成和演化的条件更加极端，我们只能观察到我们认为将成为球状星团的少数天体的综合光。因此，我们将讨论如何数值和分析方法，告知在本地宇宙中观察到的集群人口的属性，被用来开发复杂的模拟可能能够解开的遗传地图的星系形成和组装所携带的球状星团人口。
Star clusters are fundamental units of stellar feedback and unique tracers of their host galactic properties. In this review, we will first focus on their constituents, i.e. detailed insight into their stellar populations and their surrounding ionised, warm, neutral, and molecular gas. We, then, move beyond the Local Group to review star cluster populations at various evolutionary stages, and in diverse galactic environmental conditions accessible in the local Universe. At high redshift, where conditions for cluster formation and evolution are more extreme, we are only able to observe the integrated light of a handful of objects that we believe will become globular clusters. We therefore discuss how numerical and analytical methods, informed by the observed properties of cluster populations in the local Universe, are used to develop sophisticated simulations potentially capable of disentangling the genetic map of galaxy formation and assembly that is carried by globular cluster populations.