activity
19932023
most citedGlobal Relationships Among the Physical Properties of Stellar Systems

230 citations · 353 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2023★ 57 cited

The two rings of (50000) Quaoar

C. L. Pereira, B. Sicardy, B. E. Morgado +66

Quaoar is a classical Trans-Neptunian Object (TNO) with an area equivalent diameter of 1,100 km and an orbital semi-major axis of 43.3 astronomical units. Based on stellar occultat…

astro-ph1997★ 230 cited

Global Relationships Among the Physical Properties of Stellar Systems

David Burstein, Ralf Bender, Sandra Faber +1

The kappa-space three-dimensional parameter system was originally defined for the physical properties of dynamically hot galaxies. Here we define self-consistent kappa-parameters f…

astro-ph1996★ 24 cited

Filament and Shape Statistics: A Quantitative Comparison of Cold + Hot and Cold Dark Matter Cosmologies vs. CfA1 Data

Romeel Davé, Doug Hellinger, Joel Primack +2

A new class of geometric statistics for analyzing galaxy catalogs is presented. Filament statistics quantify filamentarity and planarity in large scale structure in a manner consis…

astro-ph1996★ 12 cited

The Small Scale Velocity Dispersion of Galaxies: A Comparison of Cosmological Simulations

Rachel S. Somerville, Joel R. Primack, Richard Nolthenius

The velocity dispersion of galaxies on small scales ( Mpc), , can be estimated from the anisotropy of the galaxy-galaxy correlation function in redshift sp…

astro-ph1995★ 2 cited

Filament Statistics: A Quantitative Comparison of Cold + Hot and Cold Dark Matter Cosmologies with CfA1 Data

Romeel Davé, Doug Hellinger, Richard Nolthenius +2

A new class of geometric statistics for analyzing galaxy catalogs is presented. {\it Filament statistics} quantify filamentarity and planarity in large scale structure in a manner…

astro-ph1993★ 28 cited

Galaxy Groups in Cold + Hot and CDM Universes: Comparison with CfA

Richard Nolthenius, Anatoly Klypin, Joel R. Primack

This letter presents results of new high resolution Cold + Hot Dark Matter (CHDM) and Cold Dark Matter (CDM) simulations. Properties of groups in these simulations reflect th…