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20042009
most citedThe effect of galaxy mass ratio on merger--driven starbursts

496 citations · 1.5k across the 8 of their papers we have counts for

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astro-ph2008428 cited

Galaxy Merger Morphologies and Time-Scales from Simulations of Equal-Mass Gas-Rich Disc Mergers

Jennifer M. Lotz, Patrik Jonsson, T. J. Cox +1

A key obstacle to understanding the galaxy merger rate and its role in galaxy evolution is the difficulty in constraining the merger properties and time-scales from instantaneous s…

astro-ph200873 cited

The Formation of Polar Disk Galaxies

Chris B. Brook, Fabio Governato, Thomas Quinn +5

Polar Ring Galaxies, such as NGC4650A, are a class of galaxy which have two kinematically distinct components that are inclined by almost 90 degrees to each other. These striking g…

astro-ph200742 cited

Predicting the Properties of the Remnants of Dissipative Galaxy Mergers

M. Covington, A. Dekel, T. J. Cox +2

We construct a physically motivated model for predicting the properties of the remnants of gaseous galaxy mergers, given the properties of the progenitors and the orbit. The model…

astro-ph2007496 cited

The effect of galaxy mass ratio on merger--driven starbursts

T. J. Cox, Patrik Jonsson, Rachel S. Somerville +2

We employ numerical simulations of galaxy mergers to explore the effect of galaxy mass ratio on merger--driven starbursts. Our numerical simulations include radiative cooling of ga…

astro-ph200739 cited

Dust Attenuation in Hydrodynamic Simulations of Spiral Galaxies

Miguel Rocha, Patrik Jonsson, Joel R. Primack +1

We study the effects of dust in hydrodynamic simulations of spiral galaxies when different radial metallicity gradients are assumed. SUNRISE, a Monte-Carlo radiative-transfer code,…

astro-ph200632 cited

Shapes of Stellar Systems and Dark Halos from Simulations of Galaxy Major Mergers

Gregory S. Novak, Thomas J. Cox, Joel R. Primack +2

Using a sample of 89 snapshots from 58 hydrodynamic binary galaxy major merger simulations, we find that stellar remnants are mostly oblate while dark matter halos are mostly prola…