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19972008
most citedRiding the Spiral Waves: Implications of Stellar Migration for the Properties of Galactic Disks

483 citations · 820 across the 4 of their papers we have counts for

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7 papers · 1 filter

astro-ph2008483 cited

Riding the Spiral Waves: Implications of Stellar Migration for the Properties of Galactic Disks

Rok Roškar, Victor P. Debattista, Thomas R. Quinn +2

Stars in disks of spiral galaxies are usually assumed to remain roughly at their birth radii. This assumption is built into decades of modelling of the evolution of stellar populat…

astro-ph20082 cited

Clues to Radial Migration from the Properties of Outer Disks

Rok Roškar, Victor P. Debattista, Thomas R. Quinn +3

The outer disks of galaxies present a unique laboratory for studying the process of disk formation. A considerable fraction of observed disks exhibit a break in their surface brigh…

astro-ph2007328 cited

Rapid Formation of Supermassive Black Hole Binaries in Galaxy Mergers with Gas

Lucio Mayer, Stelios Kazantzidis, Piero Madau +3

Supermassive black holes (SMBHs) are a ubiquitous component of the nuclei of galaxies. It is normally assumed that, following the merger of two massive galaxies, a SMBH binary will…

astro-ph20047 cited

Disk Galaxy Rotation Curves in Triaxial CDM Halos

E. Hayashi, J. F. Navarro, A. Jenkins +7

We use N-body hydrodynamical simulations to study the structure of disks in triaxial potentials resembling CDM halos. Our analysis focuses on the accuracy of the dark mass distribu…

astro-ph1999

The fate of LSB galaxies in clusters and the origin of the diffuse intra-cluster light

Ben Moore, George Lake, Joachim Stadel +1

We follow the evolution of disk galaxies within a cluster that forms hierarchically in a standard cold dark matter N-body simulation. At a redshift z=0.5 we select several dark mat…

astro-ph1997

The Structure and Dynamics of Cold Dark Matter Halos

Ben Moore, Sebastiano Ghigna, Fabio Governato +3

We investigate the internal structure of cold dark matter halos using high resolution N-body simulations. As the mass and force resolution are increased, halo density profiles beco…