Bulge Model
The Bulge Radial Velocity Assay

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The Team


R. Michael Rich; The University of California, Los Angeles

Christian Howard; Stratospheric Observatory for Infrared Astronomy

Andreas Koch; University of Heidelberg

Juntai Shen, Shanghai Astronomical Observatory

Hong Sheng Zhao; University of Saint Andrews

John Kormendy; The University of Texas at Austin

Roberto De Propris; Cerro Tololo Inter-American Observatory

Christian Johnson; The University of California, Los Angeles

Mario Soto; Space Telescope Science Institute, Baltimore

Livia Origlia; Osservatorio Astronomico di Bologna

Annie Robin; Observatoire de Besançon

Andrea Kunder; Cerro Tololo Inter-American Observatory

Yougang Wang; National Astronomical Observatoires, Chinese Academy of Sciences

Peter, Frinchaboy; Texas Christian University

David Reitzel; Griffith Observatory

Department of Physics and Astronomy
The Bulge Radial Velocity Assay, or BRAVA was conceived as a survey of the line-of-sight velocity distribution of red giants across the bulge, to be compared with self-consistent dynamical models.

Last updated on: 07/14/2011