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19992026
most citedGalactic star formation and accretion histories from matching galaxies to dark matter haloes

1.4k citations · 34.8k across the 266 of their papers we have counts for

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Showing 2010Show all

12 papers · 1 filter

astro-ph.CO2010★ 1.1k cited

The Atlas3D project -- I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria

Michele Cappellari, Eric Emsellem, Davor Krajnovic +23

The Atlas3D project is a multi-wavelength survey combined with a theoretical modeling effort. The observations span from the radio to the millimeter and optical, and provide multi-…

astro-ph.CO2010★ 25 cited

Disruption of Star Clusters in the Interacting Antennae Galaxies

Simon J. Karl, S. Michael Fall, Thorsten Naab

We reexamine the age distribution of star clusters in the Antennae in the context of N-body+hydrodynamical simulations of these interacting galaxies. All of the simulations that ac…

astro-ph.GA2010★ 40 cited

Galactic ménage à trois: Simulating magnetic fields in colliding galaxies

H. Kotarba, H. Lesch, K. Dolag +4

We present high resolution simulations of a multiple merger of three disk galaxies including the evolution of magnetic fields performed with the N-body/SPH code Gadget. For the fir…

astro-ph.CO2010★ 183 cited

Short-lived star-forming giant clumps in cosmological simulations of z~2 disks

Shy Genel, Thorsten Naab, Reinhard Genzel +7

Many observed massive star-forming z\approx2 galaxies are large disks that exhibit irregular morphologies, with \sim1kpc, \sim10^(8-10)Msun clumps. We present the largest sample to…

astro-ph.CO2010★ 811 cited

The Two Phases of Galaxy Formation

Ludwig Oser, Jeremiah P. Ostriker, Thorsten Naab +2

Cosmological simulations of galaxy formation appear to show a two-phase character with a rapid early phase at z>2 during which in-situ stars are formed within the galaxy from infal…

astro-ph.GA2010★ 16 cited

The Effects of X-Ray and UV Background Radiation on the Low-Mass Slope of the Galaxy Mass Function

D. C. Hambrick, J. P. Ostriker, P. H. Johansson +1

Even though the dark-matter power spectrum in the absence of biasing predicts a number density of halos n(M) ~ M^-2 (i.e. a Schechter alpha value of -2) at the low-mass end (M < 10…