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相关论文: The Formation and Evolution of Star Clusters and G…

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This review focuses on how galaxies and their globular cluster systems form. I first discuss the now fairly convincing evidence that some globular clusters form in galaxy starbursts/mergers. One way these observations are valuable is they…

天体物理学 · 物理学 2007-05-23 Stephen E. Zepf

Their ubiquity and extreme densities make star clusters probes of prime importance of galaxy evolution. Old globular clusters keep imprints of the physical conditions of their assembly in the early Universe, and younger stellar objects,…

星系天体物理 · 物理学 2018-05-02 Florent Renaud

Young stars form on a wide range of scales, producing aggregates and clusters with various degrees of gravitational self-binding. The loose aggregates have a hierarchical structure in both space and time that resembles interstellar…

天体物理学 · 物理学 2007-05-23 B. G. Elmegreen , Y. N. Efremov , R. E. Pudritz , H. Zinnecker

Globular clusters provide a unique probe of galaxy formation and evolution. Here I briefly summarize the known observational properties of globular cluster systems. One re-occurring theme is that the globular cluster systems of spirals and…

天体物理学 · 物理学 2007-05-23 Duncan A. Forbes

We present a high-resolution simulation of globular cluster formation in a galaxy merger. For the first time in such a simulation, individual star clusters are directly identified and followed on their orbits. We quantitatively compare star…

天体物理学 · 物理学 2009-11-10 Yuexing Li , Mordecai-Mark Mac Low , Ralf S. Klessen

Globular cluster systems provide valuable fossil records of the formation history of their parent galaxies. This review specifically concentrates on using color distributions of the globular cluster systems of elliptical galaxies to…

天体物理学 · 物理学 2007-05-23 Stephen E. Zepf

Understanding the formation of globular clusters will help us to constrain the evolutionary history of galaxies. For mergers on-going today, it appears that the number of newly created proto-globulars varies with the progenitor types and…

天体物理学 · 物理学 2007-05-23 Duncan Forbes

An overview of our current understanding of the formation and evolution of star clusters is given, with main emphasis on high-mass clusters. Clusters form deeply embedded within dense clouds of molecular gas. Left-over gas is cleared within…

星系天体物理 · 物理学 2015-05-14 Soeren S. Larsen

Star cluster formation is a major mode of star formation in the extreme conditions of interacting galaxies and violent starbursts. Young clusters are observed to form in a variety of such galaxies, a substantial number resembling the…

天体物理学 · 物理学 2007-05-23 P. Anders , U. Fritze--v. Alvensleben , R. de Grijs

We review recent work that investigates the formation of stellar clusters, ranging in scale from globular clusters through open clusters to the small scale aggregates of stars observed in T associations. In all cases, recent advances in…

天体物理学 · 物理学 2007-05-23 Cathie J. Clarke , Ian A. Bonnell , Lynne A. Hillenbrand

Star formation plays a central role in the evolution of galaxies and of the Universe as a whole. Studies of star-forming regions in the local universe have shown that star formation typically occurs in a clustered fashion. Building a…

In about 40% of the Local Group galaxies star clusters have been detected so far, but the census is still incomplete. The properties of these clusters are briefly reviewed, and the impact of galaxy environment on the evolution and survival…

天体物理学 · 物理学 2007-05-23 Eva K. Grebel

Globular clusters are valuable fossil records of the formation and evolution of their host galaxies. The color distribution of elliptical galaxy globular cluster systems indicates an episodic formation history, consistent with a merger…

天体物理学 · 物理学 2007-05-23 Stephen E. Zepf

We discuss some of the key open questions regarding the formation and evolution of globular clusters (GCs) during galaxy formation and assembly within a cosmological framework. The current state-of-the-art for both observations and…

Globular clusters are large and dense agglomerate of stars. At variance with smaller clusters of stars, they exhibit signs of some chemical evolution. At least for this reason, they are intermediate between open clusters and massive objects…

太阳与恒星天体物理 · 物理学 2019-11-11 Raffaele Gratton , Angela Bragaglia , Eugenio Carretta , Valentina D'Orazi , Sara Lucatello , Antonio Sollima

Young, massive star clusters are the most notable and significant end products of violent star-forming episodes triggered by galaxy collisions, mergers, and close encounters. The question remains, however, whether or not at least a fraction…

天体物理学 · 物理学 2009-11-11 Richard de Grijs

The present-day globular cluster populations of galaxies reflect the cumulative effects of billions of years of galaxy evolution via such processes as mergers, tidal stripping, accretion, and in some cases the partial or even complete…

天体物理学 · 物理学 2007-05-23 Michael J. West

In a series of three papers, we introduced a novel cluster formation model that describes the formation, growth, and disruption of star clusters in high-resolution cosmological simulations. We tested this model on a Milky Way-sized galaxy…

星系天体物理 · 物理学 2020-03-18 Hui Li , Oleg Gnedin

Mergers of gas-rich galaxies lead to gravitationally driven increases in gas pressure that can trigger intense bursts of star and cluster formation. Although star formation itself is clustered, most newborn stellar aggregates are unbound…

天体物理学 · 物理学 2007-05-23 Francois Schweizer

Globular Cluster (GC) formation seems to be a widespread mode of star formation in extreme starbursts triggered by strong interactions and mergers of massive gas-rich galaxies. We use our detailed chemically consistent evolutionary…

天体物理学 · 物理学 2015-06-10 Uta Fritze -- v. Alvensleben
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