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 (Sgr A*) is present. Our high precision N- body simulations show a good fit to the observational characteristics of the Milky Way nuclear cluster, giving further reliability to the so called migratory model for the formation of compact systems in the inner galaxy regions

Galactic nuclear cluster formation via globular cluster mergers / CAPUZZO DOLCETTA, Roberto Angelo. - In: MEMORIE DELLA SOCIETÀ ASTRONOMICA ITALIANA. - ISSN 0037-8720. - STAMPA. - 84:(2013), pp. 167-170. (Intervento presentato al convegno Reading the book of globular clusters with the lens of stellar evolution tenutosi a Monteporzio Catone (I) nel 26-28 november 2012).

Galactic nuclear cluster formation via globular cluster mergers

CAPUZZO DOLCETTA, Roberto Angelo
2013

Abstract

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 (Sgr A*) is present. Our high precision N- body simulations show a good fit to the observational characteristics of the Milky Way nuclear cluster, giving further reliability to the so called migratory model for the formation of compact systems in the inner galaxy regions
2013
Reading the book of globular clusters with the lens of stellar evolution
galaxies: nuclei; galaxies: black holes; galaxies: globular clusters; galaxies: Milky Way; N-body: simulations
04 Pubblicazione in atti di convegno::04c Atto di convegno in rivista
Galactic nuclear cluster formation via globular cluster mergers / CAPUZZO DOLCETTA, Roberto Angelo. - In: MEMORIE DELLA SOCIETÀ ASTRONOMICA ITALIANA. - ISSN 0037-8720. - STAMPA. - 84:(2013), pp. 167-170. (Intervento presentato al convegno Reading the book of globular clusters with the lens of stellar evolution tenutosi a Monteporzio Catone (I) nel 26-28 november 2012).
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/519656
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