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Globular clusters in galaxies have a mutual feedback with the environment, which is tuned by their dynamical evolution. This feedback may be the explanation of various features of both the globular cluster system and the host galaxy.…

天体物理学 · 物理学 2007-05-23 R. Capuzzo-Dolcetta

The radial distribution of globular clusters in galaxies is always less peaked to the centre than the halo stars'. Extending previous work to a sample of HST globular cluster systems in ellipticals, we evaluate the number of clusters lost…

天体物理学 · 物理学 2009-10-30 R. Capuzzo-Dolcetta , A. Tesseri

Globular cluster systems evolve, in galaxies, due to internal and external dynamics and tidal phenomena. One of the causes of evolution, dynamical friction, is responsible for the orbital decay of massive clusters into the innermost…

天体物理学 · 物理学 2009-11-10 R. Capuzzo-Dolcetta

Globular clusters (GCs) constitute a system which is evolving because of various interactions with the galactic environment. Evolution may be the explanation of many observed features of Globular Cluster Systems (GCSs); the different radial…

天体物理学 · 物理学 2007-05-23 R. Capuzzo-Dolcetta

Different types of observations, together with consistent and physical modelizations, suggest as realistic the hypothesis of enrichement of galactic nuclei by mean of massive globular clusters orbitally decayed and merged in the inner…

天体物理学 · 物理学 2008-11-26 R. Capuzzo-Dolcetta

Dynamical friction due to field stars and tidal disruption caused by a central nucleus are crucial in determining the evolution of the globular cluster system in an elliptical galaxy. In this paper I examine the possibility that some of…

天体物理学 · 物理学 2009-10-22 R. Capuzzo-Dolcetta

Giant elliptical galaxies, believed to be built from the merger of lesser galaxies, are known to house a massive black hole at their center rather than a compact star cluster. If low- and intermediate-mass galaxies do indeed partake in the…

宇宙学与河外天体物理 · 物理学 2015-05-18 Kenji Bekki , Alister W. Graham

In this paper we present the results of two detailed N-body simulations of the interaction of a sample of four massive globular clusters in the inner region of a triaxial galaxy. A full merging of the clusters takes place, leading to a…

天体物理学 · 物理学 2009-11-13 R. Capuzzo-Dolcetta , P. Miocchi

Galactic globular clusters, which are ancient building blocks of our Galaxy, represent a very interesting family of stellar systems in which some fundamental dynamical processes have taken place on time scales shorter than the age of the…

天体物理学 · 物理学 2014-10-13 G. Meylan , D. C. Heggie

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

Recent developments relevant to the formation of globular cluster systems in galaxies are discussed, including (1) The age distribution of the oldest Milky Way clusters, (2) Subgroups and possible accretion and merger remnants in the…

天体物理学 · 物理学 2007-05-23 W. E. Harris

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

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

The decay of globular clusters to the center of their mother galaxy corresponds to carrying a quantity of mass sufficient to sustain the gravitational activity of a small pre-existing nucleus and to accrete it in a significant way. This is…

天体物理学 · 物理学 2007-05-23 R. Capuzzo-Dolcetta , P. Miocchi

We study the evolution of the galactic globular cluster system to determine its initial mass-function and the fraction of halo stars that could have come from disrupted globular clusters. We study the cluster evolution under the influence…

天体物理学 · 物理学 2007-05-23 H. Baumgardt

The evolution of galaxies is driven strongly by dynamical processes including internal instabilities, tidal interactions and mergers. The cluster environment is a useful laboratory for studying these effects. I present recent results on…

天体物理学 · 物理学 2007-05-23 John Dubinski

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

In this paper we address the issue of the origin of some observational properties of the galactic globular cluster system. After a preliminary study of some general properties of the main evolutionary processes, we investigate the evolution…

天体物理学 · 物理学 2015-06-24 E. Vesperini

Some factors connecting the evolutionary histories of galaxies with the characteristics of their cluster systems are reviewed. Unanswered questions include: How is one to understand the observation that some globular cluster systems have…

天体物理学 · 物理学 2007-05-23 Sidney van den Bergh

We revisit the hypothesis that dense galactic nuclei are formed from inspiraling globular clusters. Recent advances in understanding of the continuous formation of globular clusters over cosmic time and the concurrent evolution of the…

宇宙学与河外天体物理 · 物理学 2015-06-16 Oleg Y. Gnedin , Jeremiah P. Ostriker , Scott Tremaine
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