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  • Models of the origin of young stars in the Galactic Centre are facing various problems. The most promising scenario of the star formation in a thin self-gravitating disc naturally forms stars on coherently rotating orbits, but it fails to explain the origin of several tens of stars that evidently do not belong to any of the disc-like structures in the GC. One possible solution lies in rather complicated initial conditions, assuming at least two infalling and interacting gas clouds. We present alternative solution showing that a single thin stellar disc may have given birth to all young stars in the GC. The outliers are explained as stars that have been stripped from the parent structure due to the gravitational interaction with the gaseous circum-nuclear disc.
  • Models of the origin of young stars in the Galactic Centre are facing various problems. The most promising scenario of the star formation in a thin self-gravitating disc naturally forms stars on coherently rotating orbits, but it fails to explain the origin of several tens of stars that evidently do not belong to any of the disc-like structures in the GC. One possible solution lies in rather complicated initial conditions, assuming at least two infalling and interacting gas clouds. We present alternative solution showing that a single thin stellar disc may have given birth to all young stars in the GC. The outliers are explained as stars that have been stripped from the parent structure due to the gravitational interaction with the gaseous circum-nuclear disc. (en)
Title
  • Stellar Disc - Dynamical Evolution in a Perturbed Potential
  • Stellar Disc - Dynamical Evolution in a Perturbed Potential (en)
skos:prefLabel
  • Stellar Disc - Dynamical Evolution in a Perturbed Potential
  • Stellar Disc - Dynamical Evolution in a Perturbed Potential (en)
skos:notation
  • RIV/00216208:11320/11:10105305!RIV12-MSM-11320___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • Z(MSM0021620860)
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
  • 232338
http://linked.open...ai/riv/idVysledku
  • RIV/00216208:11320/11:10105305
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • potential; stellar disc (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...ontrolniKodProRIV
  • [AB5BFB45645F]
http://linked.open...v/mistoKonaniAkce
  • Shanghai, PEOPLES R CHINA
http://linked.open...i/riv/mistoVydani
  • 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA
http://linked.open...i/riv/nazevZdroje
  • GALACTIC CENTER: A WINDOW TO THE NUCLEAR ENVIRONMENT OF DISK GALAXIES
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...UplatneniVysledku
http://linked.open...iv/tvurceVysledku
  • Šubr, Ladislav
http://linked.open...vavai/riv/typAkce
http://linked.open...ain/vavai/riv/wos
  • 000291890200046
http://linked.open.../riv/zahajeniAkce
http://linked.open...n/vavai/riv/zamer
number of pages
http://purl.org/ne...btex#hasPublisher
  • ASTRONOMICAL SOC PACIFIC
https://schema.org/isbn
  • 978-1-58381-758-2
http://localhost/t...ganizacniJednotka
  • 11320
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