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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…

星系天体物理 · 物理学 2010-01-29 Rainer Schoedel

The nuclear star cluster of the Milky Way is a unique target in the Universe. Contrary to extragalactic nuclear star clusters, using current technology it can be resolved into tens of thousands of individual stars. This allows us to study…

天体物理学 · 物理学 2014-11-18 R. Schoedel , D. Merritt , A. Eckart

This article intends to provide a concise overview, from an observational point-of-view, of the current state of our knowledge of the most relevant properties of the Milky Way's nuclear star cluster (MWNSC). The MWNSC appears to be a…

星系天体物理 · 物理学 2015-06-23 R. Schödel , A. Feldmeier , N. Neumayer , L. Meyer , S. Yelda

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…

星系天体物理 · 物理学 2011-07-05 Roberto Capuzzo-Dolcetta , Fabio Antonini , Alessandra Mastrobuono-Battisti

This chapter provides a detailed overview of Sagittarius A* (Sgr A*), the supermassive black hole at the center of the Milky Way, located in the dense Galactic Center region approximately 8 kpc from Earth. Despite its relatively low…

星系天体物理 · 物理学 2025-03-27 Anna Ciurlo , Mark R. Morris

The Galactic Center is an excellent laboratory for studying phenomena and physical processes that may be occurring in many other galactic nuclei. The Center of our Milky Way is by far the closest galactic nucleus, and observations with…

星系天体物理 · 物理学 2015-05-19 Reinhard Genzel , Frank Eisenhauer , Stefan Gillessen

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…

星系天体物理 · 物理学 2015-03-19 Alessandra Mastrobuono-Battisti , Roberto Capuzzo-Dolcetta

The region bounded by the inner tens of light years at the center of the Milky Way contains five principal components that coexist within the central deep gravitational potential well. These constituents are a black hole candidate (Sgr~A*)…

天体物理学 · 物理学 2015-06-24 F. Yusef-Zade , F. Melia , M. Wardle

In the past decade high resolution measurements in the infrared employing adaptive optics imaging on 10m telescopes have allowed determining the three dimensional orbits stars within ten light hours of the compact radio source at the center…

天体物理学 · 物理学 2010-05-19 R. Genzel , V. Karas

The center of the Milky Way hosts a massive black hole. The observational evidence for its existence is overwhelming. The compact radio source Sgr A* has been associated with a black hole since its discovery. In the last decade,…

星系天体物理 · 物理学 2010-02-08 S. Gillessen , F. Eisenhauer , H. Bartko , K. Dodds-Eden , T. K. Fritz , O. Pfuhl , T. Ott , R. Genzel

The centre of the Milky Way is occupied by a nuclear star cluster, which contains the supermassive black hole Sgr A*. The cluster is embedded in the larger surrounding nuclear stellar disc. These three components dominate the mass budget of…

星系天体物理 · 物理学 2026-05-07 A. Feldmeier-Krause , T. I. Maindl , G. van den Ven , S. Thater , P. Jethwa , I. Breda

A massive black hole resides in the center of most, perhaps all galaxies. The one in the center of our home galaxy, the Milky Way, provides a uniquely accessible laboratory for studying in detail the connections and interactions between a…

天体物理学 · 物理学 2009-11-13 Tal Alexander

Nuclear star clusters (NSCs) are located at the photometric and dynamical centers of the majority of galaxies. They are among the densest star clusters in the Universe. The NSC in the Milky Way is the only object of this class that can be…

星系天体物理 · 物理学 2015-05-13 R. Schoedel , D. Merritt , A. Eckart

The black hole at the center of our Milky Way Galaxy -- the Galactic Black Hole, or GBH -- is a rather modest representative of its class. With a mass of 4 x 10^6 solar masses, it is well over a thousand times less massive than the most…

星系天体物理 · 物理学 2023-02-20 Mark R. Morris

With its extreme density of stars and stellar remnants, dense young massive clusters, high specific star formation rate, intense radiation field, high magnetic field strength, and properties of the interstellar medium that resemble those in…

The Milky Way is the only galaxy for which we can resolve individual stars at all evolutionary phases, from the Galactic center to the outskirt. The last decade, thanks to the advent of near IR detectors and 8 meter class telescopes, has…

天体物理学 · 物理学 2009-11-13 Dante Minniti , Manuela Zoccali

Recent measurements, of the velocities of stars near the center of the Milky Way have provided the strongest evidence for the presence of a supermassive black hole in a galaxy, but the observational uncertainties poorly constrain many of…

天体物理学 · 物理学 2009-10-31 A. Ghez , M. Morris , E. E. Becklin , T. Kremenek , A. Tanner

This is a pedagogical review of recent results on the interactions of central massive black holes with stars very near them, focused on the black hole in the center of the Milky Way. Table of contents: [1] Introduction [2] Stellar dynamics…

天体物理学 · 物理学 2007-05-23 Tal Alexander

The Galactic Center is the closest galactic nucleus that can be studied with unprecedented angular resolution and sensitivity. We summarize recent basic observational results on Sagittarius A* and the conditions for star formation in the…

This review outlines the observations that now provide an overwhelming scientific case that the center of our Milky Way Galaxy harbors a supermassive black hole. Observations at infrared wavelength trace stars that orbit about a common…

天体物理学 · 物理学 2009-07-22 Mark J. Reid
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