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19992007
most citedOrigin of Abundance Inhomogeneity in Globular Clusters

93 citations · 115 across the 5 of their papers we have counts for

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astro-ph200793 cited

Origin of Abundance Inhomogeneity in Globular Clusters

K. Bekki, S. W. Campbell, J. C. Lattanzio +1

We numerically investigate abundance properties of the Galactic globular clusters (GCs) by adopting a new ``external pollution'' scenario. In this framework, GCs are assumed to ori…

astro-ph200720 cited

On the Origin of Mass--Metallicity Relations, Blue Tilts, and Scaling Relations for Metal-poor Globular Cluster Systems

K. Bekki, H. Yahagi, D. A. Forbes

We investigate formation processes and physical properties of globular cluster systems (GCSs) in galaxies based on high-resolution cosmological simulations with globular clusters.…

astro-ph20072 cited

Probing clumpy pasts of galaxies from AGB stars

K. Bekki, M. -R. L. Cioni

Recent morphological studies of galaxies by the {\it Hubble Space Telescope (HST)} have revealed that actively star-forming galaxies at intermediate and high redshifts (

astro-ph2003

Evolution of galaxies in triaxial halos with figure rotation

K. Bekki, K. C. Freeman

Firstly, we demonstrate that unusually large outer HI spiral arms observed in NGC 2915 can form in an extended gas disk embedded in a massive triaxial dark matter halo with slow fi…

astro-ph2003

Galaxy threshing and the origin of intracluster stellar objects

K. Bekki, W. J. Couch, M. D. Drinkwater +1

We numerically investigate dynamical evolution of non-nucleated dwarf elliptical/spiral galaxies (dE) and nucleated ones (dE,Ns) in clusters of galaxies in order to understand the…

astro-ph2003

Formation of globular clusters in galaxy mergers

Kenji Bekki, Warrick J. Couch, Duncan A. Forbes +1

Our numerical simulations first demonstrate that the pressure of ISM in a major merger becomes so high ( K ) that GMCs in the merger can coll…