. . "1"^^ . "0004-6361" . . "RIV/67985815:_____/12:00387362!RIV13-GA0-67985815" . "[A85BC4F2660E]" . . "000304390900064" . . "Carraro, G." . "4"^^ . "157119" . "541" . . . . "April" . . "The origin and orbit of the old, metal-rich, open cluster NGC 6791. Insights from kinematics" . "galaxy; kinematics and dynamics; open clusters and associations"@en . . "The origin and orbit of the old, metal-rich, open cluster NGC 6791. Insights from kinematics"@en . "RIV/67985815:_____/12:00387362" . . . . "P(GD205/08/H005), P(LC06014), Z(AV0Z10030501)" . "Astronomy & Astrophysics" . . . . "Minchev, I." . . "Jungwiert, Bruno" . "The origin and orbit of the old, metal-rich, open cluster NGC 6791. Insights from kinematics"@en . "FR - Francouzsk\u00E1 republika" . "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\u2019s orbit and investigate the possible migration processes that may have displaced NGC\u20096791 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\u20096791 from the inner disk (galocentric radii of 3\u20135\u2009kpc) 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." . "10.1051/0004-6361/201117347" . . "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\u2019s orbit and investigate the possible migration processes that may have displaced NGC\u20096791 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\u20096791 from the inner disk (galocentric radii of 3\u20135\u2009kpc) 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 . . "J\u00EDlkov\u00E1, L." . "11"^^ . "The origin and orbit of the old, metal-rich, open cluster NGC 6791. Insights from kinematics" .