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Dynamical evolution of dense star clusters in galactic nuclei

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F14%3A10287739" target="_blank" >RIV/00216208:11320/14:10287739 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1017/S1743921314000647" target="_blank" >http://dx.doi.org/10.1017/S1743921314000647</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1017/S1743921314000647" target="_blank" >10.1017/S1743921314000647</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Dynamical evolution of dense star clusters in galactic nuclei

  • Original language description

    By means of direct numerical N-body modeling, we investigate the orbital evolution of an initially thin, central mass dominated stellar disk. We include the perturbative gravitational influence of an extended spherically symmetric star cluster and the mutual gravitational interaction of the stars within the disk. Our results show that the two-body relaxation of the disk leads to significant changes of its radial density profile. In particular, the disk naturally evolves, for a variety of initial configurations, a similar broken power-law surface density profile. Hence, it appears that the single power-law surface density profile PROPORTIONAL TOR -2 suggested by various authors to describe the young stellar disk observed in the Sgr A* region does not match theoretical expectations.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/LD12065" target="_blank" >LD12065: Black holes and their environment</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2014

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Article name in the collection

    The Galactic Center: Feeding and Feedback in a Normal Galactic Nucleus

  • ISBN

    978-1-107-04461-6

  • ISSN

    1743-9213

  • e-ISSN

  • Number of pages

    3

  • Pages from-to

    235-237

  • Publisher name

    Cambridge University Press

  • Place of publication

    Cambridge, UK

  • Event location

    Santa Fe, NM, USA

  • Event date

    Sep 30, 2013

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article