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  • 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.
  • 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. (en)
Title
  • Dynamical evolution of dense star clusters in galactic nuclei
  • Dynamical evolution of dense star clusters in galactic nuclei (en)
skos:prefLabel
  • Dynamical evolution of dense star clusters in galactic nuclei
  • Dynamical evolution of dense star clusters in galactic nuclei (en)
skos:notation
  • RIV/00216208:11320/14:10287739!RIV15-MSM-11320___
http://linked.open...avai/riv/aktivita
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  • P(LD12065)
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 12693
http://linked.open...ai/riv/idVysledku
  • RIV/00216208:11320/14:10287739
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • Galaxy: nucleus; stellar dynamics; methods: n-body simulations (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...ontrolniKodProRIV
  • [904F587664BA]
http://linked.open...v/mistoKonaniAkce
  • Santa Fe, NM, USA
http://linked.open...i/riv/mistoVydani
  • Cambridge, UK
http://linked.open...i/riv/nazevZdroje
  • The Galactic Center: Feeding and Feedback in a Normal Galactic Nucleus
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...iv/tvurceVysledku
  • Šubr, Ladislav
  • Haas, Jaroslav
http://linked.open...vavai/riv/typAkce
http://linked.open.../riv/zahajeniAkce
issn
  • 1743-9213
number of pages
http://bibframe.org/vocab/doi
  • 10.1017/S1743921314000647
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  • Cambridge University Press
https://schema.org/isbn
  • 978-1-107-04461-6
http://localhost/t...ganizacniJednotka
  • 11320
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