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Related papers: Nuclear Star Clusters across the Hubble Sequence

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The centers of most galaxies in the local universe are occupied by compact, barely resolved sources. Based on their structural properties, position in the fundamental plane, and integrated spectra, these sources clearly have a stellar…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Torsten Boeker

HST observations have revealed that compact sources exist at the centers of many, maybe even most, galaxies across the Hubble sequence. These sources are called "nuclei" or also "nuclear star clusters" (NCs), given that their structural…

We review the current knowledge about nuclear star clusters (NSCs), the spectacularly dense and massive assemblies of stars found at the centers of most galaxies. Recent observational and theoretical work suggest that many NSC properties,…

Astrophysics of Galaxies · Physics 2020-07-15 Nadine Neumayer , Anil Seth , Torsten Boeker

Nuclear star clusters are found at the centers of most galaxies. They are the densest stellar systems in the Universe, and thus have unique and interesting stellar dynamics. We review how common nuclear star clusters are in galaxies of…

Astrophysics of Galaxies · Physics 2020-03-18 Anil C. Seth , Nadine Neumayer , Torsten Boeker

Nuclear star clusters are among the densest stellar systems known and are common in both early- and late-type galaxies. They exhibit scaling relations with their host galaxy which may be related to those of supermassive black holes. These…

Astrophysics of Galaxies · Physics 2015-12-09 David R. Cole , Victor P. Debattista

Nuclear stellar cluster (NSCs) are known to exist around massive black holes (MBHs) in galactic nuclei. Two formation scenarios were suggested for their origin: Build-up of NSCs and Continuous in-situ star-formation. Here we study the…

Astrophysics of Galaxies · Physics 2017-08-23 Danor Aharon , Hagai B. Perets

Nuclear Star Clusters are observed at the center of many galaxies. In particular in the center of the Milky Way the Nuclear Star Cluster coexists with a cen- tral supermassive black hole. The origin of these clusters is still unknown; a…

Astrophysics of Galaxies · Physics 2015-03-19 Alessandra Mastrobuono-Battisti , Roberto Capuzzo-Dolcetta

The centers of stellar spheroids are often marked by the presence of nucleated central regions, called nuclear star clusters (NSCs). The origin of NSCs is still unclear. Here we investigate the possibility that NSCs originate from the…

Astrophysics of Galaxies · Physics 2015-06-05 Fabio Antonini

In the center of the Milky Way, as well as in many other galaxies, a compact star cluster around a very massive black hole is observed. One of the possible explanations for the formation of such Nuclear Star Clusters is based on the…

Astrophysics of Galaxies · Physics 2011-07-05 Roberto Capuzzo-Dolcetta , Fabio Antonini , Alessandra Mastrobuono-Battisti

This is an overview of nuclear star cluster observations, covering their structure, stellar populations, kinematics and possible connection to black holes at the centers of galaxies.

Cosmology and Nongalactic Astrophysics · Physics 2012-11-09 Nadine Neumayer

Nuclear star clusters (NSCs) are the densest stellar systems in the Universe and are found in the centres of all types of galaxies. They are thought to form via mergers of star clusters such as ancient globular clusters (GCs) that spiral to…

A large fraction of bulgeless disk galaxies contain young compact stellar systems at their centers, in spite of the local gravitational stability of these disks. We evaluate two contrasting hypotheses for the origin of the nuclear star…

Astrophysics · Physics 2009-11-10 Milos Milosavljevic

The ACS Virgo cluster survey by Cote' and collaborators shows the presence of compact nuclei at the photocenters of many early-type galaxies. It is argued that they are the low-mass counterparts of nuclei hosting Super Massive Black Holes…

Astrophysics · Physics 2007-09-05 R. Capuzzo-Dolcetta , P. Miocchi

We study galaxies that host both nuclear star clusters and active galactic nuclei (AGN) implying the presence of a massive black hole. We select a sample of 176 galaxies with previously detected nuclear star clusters that range from…

Astrophysics · Physics 2009-11-13 Anil Seth , Marcel Agueros , Duane Lee , Antara Basu-Zych

Nuclear stellar cluster (NSCs) are known to exist around massive black holes (MBHs) in galactic nuclei. They are thought to have formed through in-situ star formation following gas inflow to the nucleus of the galaxy and/or through the…

Astrophysics of Galaxies · Physics 2015-06-18 Hagai B. Perets , Alessandra Mastrobuono-Battisti

Nuclear stellar cluster (NSCs) are known to exist around massive black holes (MBHs) in galactic nuclei. Two formation scenarios were suggested for their origin: (1) Build-up of NSCs from consecutive infall of stellar cluster and (2)…

Astrophysics of Galaxies · Physics 2015-06-22 Danor Aharon , Hagai B. Perets

We apply the idea that dense stellar systems in the central region of galaxies are formed via globular cluster mergers to the formation of the nuclear star cluster of the Milky Way, where a massive black hole is present. Our high precision…

Astrophysics of Galaxies · Physics 2013-01-15 Roberto Capuzzo-Dolcetta

Nuclear star clusters are located at the dynamical centers of the majority of galaxies. They are usually the densest and most massive star cluster in their host galaxy. In this article, I will give a brief overview of our current knowledge…

Astrophysics of Galaxies · Physics 2010-01-29 Rainer Schoedel

Nuclear star clusters (NSCs) are the densest stellar systems in the Universe. They can be found at the center of all galaxy types, but tend to favor galaxies of intermediate stellar mass around 10$^9\,$M$_{\odot}$[1, 2]. Currently, two main…

The origin of the Nuclear Star Cluster in the centre of our Galaxy is still unknown. One possibility is that it formed after the disruption of stellar clusters that spiralled into the Galactic Centre due to dynamical friction. We trace the…

Astrophysics of Galaxies · Physics 2017-11-20 F. Abbate , A. Mastrobuono-Battisti , M. Colpi , A. Possenti , A. C. Sippel , M. Dotti
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