About: The origin and orbit of the old, metal-rich, open cluster NGC 6791. Insights from kinematics     Goto   Sponge   NotDistinct   Permalink

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  • One possible scenario is that the cluster formed close to the Galactic Center and later migrated outward to its current location. In this work we study the cluster’s orbit and investigate the possible migration processes that may have displaced NGC 6791 to its present-day position, under the assumption that it actually formed in the inner disk. We find that a model that incorporates a strong bar and spiral arm perturbations can indeed be responsible for the migration of NGC 6791 from the inner disk (galocentric radii of 3–5 kpc) to its present-day location. Such a model can provide orbital parameters that are close enough to the observed ones. However, the probability of this scenario as it results from our investigations is very low.
  • One possible scenario is that the cluster formed close to the Galactic Center and later migrated outward to its current location. In this work we study the cluster’s orbit and investigate the possible migration processes that may have displaced NGC 6791 to its present-day position, under the assumption that it actually formed in the inner disk. We find that a model that incorporates a strong bar and spiral arm perturbations can indeed be responsible for the migration of NGC 6791 from the inner disk (galocentric radii of 3–5 kpc) to its present-day location. Such a model can provide orbital parameters that are close enough to the observed ones. However, the probability of this scenario as it results from our investigations is very low. (en)
Title
  • The origin and orbit of the old, metal-rich, open cluster NGC 6791. Insights from kinematics
  • The origin and orbit of the old, metal-rich, open cluster NGC 6791. Insights from kinematics (en)
skos:prefLabel
  • The origin and orbit of the old, metal-rich, open cluster NGC 6791. Insights from kinematics
  • The origin and orbit of the old, metal-rich, open cluster NGC 6791. Insights from kinematics (en)
skos:notation
  • RIV/67985815:_____/12:00387362!RIV13-GA0-67985815
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GD205/08/H005), P(LC06014), Z(AV0Z10030501)
http://linked.open...iv/cisloPeriodika
  • April
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
  • 157119
http://linked.open...ai/riv/idVysledku
  • RIV/67985815:_____/12:00387362
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • galaxy; kinematics and dynamics; open clusters and associations (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • FR - Francouzská republika
http://linked.open...ontrolniKodProRIV
  • [A85BC4F2660E]
http://linked.open...i/riv/nazevZdroje
  • Astronomy & Astrophysics
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...v/svazekPeriodika
  • 541
http://linked.open...iv/tvurceVysledku
  • Jungwiert, Bruno
  • Jílková, L.
  • Carraro, G.
  • Minchev, I.
http://linked.open...ain/vavai/riv/wos
  • 000304390900064
http://linked.open...n/vavai/riv/zamer
issn
  • 0004-6361
number of pages
http://bibframe.org/vocab/doi
  • 10.1051/0004-6361/201117347
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