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The origin and orbit of the old, metal-rich, open cluster NGC 6791 Insights from kinematics

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F12%3A10129339" target="_blank" >RIV/00216208:11320/12:10129339 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/12:00387362 RIV/00216224:14310/12:00057987

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201117347" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201117347</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201117347" target="_blank" >10.1051/0004-6361/201117347</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    The origin and orbit of the old, metal-rich, open cluster NGC 6791 Insights from kinematics

  • Original language description

    Context. NGC6791 is a unique stellar system among Galactic open clusters, which is at the same time one of the oldest open clusters and the most metal rich. It is located inside the solar circle, harbors a large population of binary stars, and possibly experienced prolonged star formation. The combination of all these properties is puzzling and poses the intriguing question of its origin. Aims. 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. Methods. To thisaim we performed integrations of NGC6791's orbit in a potential consistent with the main Milky Way parameters. In addition to analytical expressions for halo, bulge and disk, we also consider the effect of bar and spiral arm perturbations

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

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

Others

  • Publication year

    2012

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astronomy and Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

  • Volume of the periodical

    541

  • Issue of the periodical within the volume

    květen

  • Country of publishing house

    DE - GERMANY

  • Number of pages

    11

  • Pages from-to

  • UT code for WoS article

    000304390900064

  • EID of the result in the Scopus database