activity
20072026
most citedAn Infrared Survey of Brightest Cluster Galaxies. II: Why are Some Brightest Cluster Galaxies Forming Stars?

274 citations · 4.5k across the 137 of their papers we have counts for

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Showing astro-ph.COShow all

6 papers · 1 filter

astro-ph.CO2013★ 69 cited

Dynamical Modeling of Galaxy Mergers using Identikit

G. C. Privon, J. E. Barnes, A. S. Evans +5

We present dynamical models of four interacting systems: NGC 5257/8, The Mice, the Antennae, and NGC 2623. The parameter space of the encounters are constrained using the Identikit…

astro-ph.CO2013★ 70 cited

Hubble Space Telescope ACS Imaging of the GOALS Sample: Quantitative Structural Properties of Nearby Luminous Infrared Galaxies with L_IR > 10^{11.4} L_sun

D. -C. Kim, A. S. Evans, T. Vavilkin +11

A {\it Hubble Space Telescope} ({\it HST}) / Advanced Camera for Surveys (ACS) study of the structural properties of 85 luminous and ultraluminous ( L$_\odo…

astro-ph.CO2012★ 35 cited

Modeling the Infrared Emission in Cygnus A

G. C. Privon, S. A. Baum, C. P. O'Dea +4

We present new Spitzer IRS spectroscopy of Cygnus A, one of the most luminous radio sources in the local universe. Data on the inner 20" are combined with new reductions of MIPS an…

astro-ph.CO2011

Experiments With IDENTIKIT

Joshua E. Barnes, George C. Privon

IDENTIKIT was originally developed as a fast approximate scheme for modeling the tidal morphology and kinematics of disk galaxy encounters and mergers. In this form, it was first u…

astro-ph.CO2011★ 49 cited

Complex Radio Spectral Energy Distributions in Luminous and Ultraluminous Infrared Galaxies

Adam K. Leroy, Aaron S. Evans, Emmanuel Momjian +11

We use the Expanded Very Large Array to image radio continuum emission from local luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) in 1 GHz windows centered at 4.7,…

astro-ph.CO2009

Modeling the Infrared Emission from Cygnus A

G. C. Privon

The Spitzer Space Telescope provides a unique view of the Universe at infrared wavelengths. Improved sensitivity and angular resolution over previous missions enable detailed studi…