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most citedAt the heart of the matter: the origin of bulgeless dwarf galaxies and Dark Matter cores

1k citations · 1.5k across the 11 of their papers we have counts for

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astro-ph2005★ 152 cited

Is there Evidence for Flat Cores in the Halos of Dwarf Galaxies?: The Case of NGC 3109 and NGC 6822

Octavio Valenzuela, George Rhee, Anatoly Klypin +4

Two well studied dwarf galaxies -- NGC 3109 and NGC 6822 -- present some of the strongest observational support for a flat core at the center of galactic dark matter (DM) halos. We…

astro-ph2003★ 123 cited

The rotation curves of dwarf galaxies: a problem for Cold Dark Matter?

George Rhee, Octavio Valenzuela, Anatoly Klypin +2

We address the issue of accuracy in recovering density profiles from observations of rotation curves of galaxies. We ``observe'' and analyze our models in much the same way as obse…

astro-ph2001★ 21 cited

A Study of 3CR Radio Galaxies from z = 0.15 to 0.65. I. Evidence for an Evolutionary Relationship Between Quasars and Radio Galaxies

Michael Harvanek, E. Ellingson, John T. Stocke

Deep optical images have been gathered for a nearly complete sample of radio galaxies from the Revised 3rd Cambridge (3CR) Catalog in the redshift range 0.15 < z < 0.65. Total and…

astro-ph1998

The ESO Nearby Abell Cluster Survey: Kinematics of Galaxies in Clusters

A. Biviano, A. Mazure, C. Adami +4

We summarize several results based on the velocity data-set for cluster galaxies provided by ENACS (the ESO Nearby Abell Cluster Survey). We describe the distribution of velocity d…

astro-ph1997

The Fundamental Plane of clusters of galaxies

C. Adami, A. Mazure, A. Biviano +2

We have used the ESO Nearby Abell Cluster Survey (ENACS) in combination with the Cosmos Galaxy Catalogue, to investigate the existence of a Fundamental Plane (FP) for rich clusters…

astro-ph1997★ 43 cited

Improved Parameters and New Lensed Features for Q0957+561 from WFPC2 Imaging

Gary Bernstein, Philippe Fischer, J. Anthony Tyson +1

New HST WFPC2 observations of the lensed double QSO 0957+561 will allow improved constraints on the lens mass distribution and hence will improve the derived value of H. We fir…