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
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Czech description
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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
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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
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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
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UT code for WoS article
000304390900064
EID of the result in the Scopus database
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