FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2047172810> ?p ?o ?g. }

• W2047172810 endingPage "420" @default.
• W2047172810 startingPage "406" @default.
• W2047172810 abstract "HIRES on the Keck I telescope has been used to measure the first radial velocities for stars belonging to eleven, heavily-reddened globular clusters in the direction of the inner Galaxy. The question of kinematic substructuring among the Galactic globular cluster system is investigated using an updated catalog of globular cluster distances, metallicities and velocities. It is found that the population of metal-rich globular clusters shows significant rotation at all Galactocentric radii. For the metal-rich clusters within 4 kpc of the Galactic center, the measured rotation velocity and line-of-sight velocity dispersion are similar to those of bulge field stars. We investigate claims that the metal-rich clusters are associated with the central Galactic bar by comparing the kinematics of the innermost clusters to that of the atomic hydrogen in the inner Galaxy. The longitude-velocity diagram of both metal-rich and metal-poor clusters bears a remarkable similarity to that of the gas, including the same non-circular motions which have traditionally been interpreted as evidence for a Galactic bar, or, alternatively, a non-axisymmetric bulge. However, uncertainties in the existing three-dimensional Galactocentric positions for most of the clusters do not yet allow an unambiguous discrimination between the competing scenarios of membership in a rigidly rotating bar, or in a bulge which is an oblate isotropic rotator. We conclude that the majority of metal-rich clusters within the central 4 kpc of the Galaxy are probably associated with the bulge/bar, and not the thick disk. (ABRIDGED)" @default.
• W2047172810 created "2016-06-24" @default.
• W2047172810 creator A5042429783 @default.
• W2047172810 date "1999-07-01" @default.
• W2047172810 modified "2023-09-23" @default.
• W2047172810 title "Kinematics of the Galactic Globular Cluster System: New Radial Velocities for Clusters in the Direction of the Inner Galaxy" @default.
• W2047172810 cites W1966714030 @default.
• W2047172810 cites W1967235714 @default.
• W2047172810 cites W1976666257 @default.
• W2047172810 cites W1980350013 @default.
• W2047172810 cites W1987981208 @default.
• W2047172810 cites W1988006098 @default.
• W2047172810 cites W1989139522 @default.
• W2047172810 cites W1993244035 @default.
• W2047172810 cites W1998883670 @default.
• W2047172810 cites W2001219150 @default.
• W2047172810 cites W2003236861 @default.
• W2047172810 cites W2007725308 @default.
• W2047172810 cites W2012980544 @default.
• W2047172810 cites W2022708325 @default.
• W2047172810 cites W2026495941 @default.
• W2047172810 cites W2032927073 @default.
• W2047172810 cites W2035620374 @default.
• W2047172810 cites W2039088976 @default.
• W2047172810 cites W2040196902 @default.
• W2047172810 cites W2041508062 @default.
• W2047172810 cites W2051924683 @default.
• W2047172810 cites W2057696957 @default.
• W2047172810 cites W2058475504 @default.
• W2047172810 cites W2060958009 @default.
• W2047172810 cites W2066406099 @default.
• W2047172810 cites W2067239832 @default.
• W2047172810 cites W2068153271 @default.
• W2047172810 cites W2069942795 @default.
• W2047172810 cites W2074571006 @default.
• W2047172810 cites W2081554211 @default.
• W2047172810 cites W2081926648 @default.
• W2047172810 cites W2085831048 @default.
• W2047172810 cites W2085887670 @default.
• W2047172810 cites W2091452000 @default.
• W2047172810 cites W2092586787 @default.
• W2047172810 cites W2105515852 @default.
• W2047172810 cites W2114602299 @default.
• W2047172810 cites W2153258189 @default.
• W2047172810 cites W2167514609 @default.
• W2047172810 cites W2170825263 @default.
• W2047172810 cites W2599734048 @default.
• W2047172810 cites W4233763166 @default.
• W2047172810 cites W4254936553 @default.
• W2047172810 cites W94000490 @default.
• W2047172810 cites W95707854 @default.
• W2047172810 doi "https://doi.org/10.1086/300930" @default.
• W2047172810 hasPublicationYear "1999" @default.
• W2047172810 type Work @default.
• W2047172810 sameAs 2047172810 @default.
• W2047172810 citedByCount "120" @default.
• W2047172810 countsByYear W20471728102012 @default.
• W2047172810 countsByYear W20471728102013 @default.
• W2047172810 countsByYear W20471728102014 @default.
• W2047172810 countsByYear W20471728102015 @default.
• W2047172810 countsByYear W20471728102016 @default.
• W2047172810 countsByYear W20471728102017 @default.
• W2047172810 countsByYear W20471728102018 @default.
• W2047172810 countsByYear W20471728102019 @default.
• W2047172810 countsByYear W20471728102020 @default.
• W2047172810 countsByYear W20471728102021 @default.
• W2047172810 countsByYear W20471728102022 @default.
• W2047172810 countsByYear W20471728102023 @default.
• W2047172810 crossrefType "journal-article" @default.
• W2047172810 hasAuthorship W2047172810A5042429783 @default.
• W2047172810 hasBestOaLocation W20471728102 @default.
• W2047172810 hasConcept C10767094 @default.
• W2047172810 hasConcept C113461152 @default.
• W2047172810 hasConcept C121332964 @default.
• W2047172810 hasConcept C127529279 @default.
• W2047172810 hasConcept C1276947 @default.
• W2047172810 hasConcept C132552067 @default.
• W2047172810 hasConcept C150846664 @default.
• W2047172810 hasConcept C37119246 @default.
• W2047172810 hasConcept C41074950 @default.
• W2047172810 hasConcept C44870925 @default.
• W2047172810 hasConcept C48393594 @default.
• W2047172810 hasConcept C98444146 @default.
• W2047172810 hasConceptScore W2047172810C10767094 @default.
• W2047172810 hasConceptScore W2047172810C113461152 @default.
• W2047172810 hasConceptScore W2047172810C121332964 @default.
• W2047172810 hasConceptScore W2047172810C127529279 @default.
• W2047172810 hasConceptScore W2047172810C1276947 @default.
• W2047172810 hasConceptScore W2047172810C132552067 @default.
• W2047172810 hasConceptScore W2047172810C150846664 @default.
• W2047172810 hasConceptScore W2047172810C37119246 @default.
• W2047172810 hasConceptScore W2047172810C41074950 @default.
• W2047172810 hasConceptScore W2047172810C44870925 @default.
• W2047172810 hasConceptScore W2047172810C48393594 @default.
• W2047172810 hasConceptScore W2047172810C98444146 @default.
• W2047172810 hasIssue "1" @default.
• W2047172810 hasLocation W20471728101 @default.
• W2047172810 hasLocation W20471728102 @default.

• next