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Faculty Research

  • Andrea Ghez and her collaborators are carrying out a diffraction-limited study of the Galaxy's central stellar cluster. This program has provided strong evidence for a supermassive black hole at the center of the Milky Way and is continuing to study the environs of this region. See the UCLA Galactic Center Research pages for more information.
  • Mark Morris studies the fate of star clusters at the Galactic center, and is trying to determine the character and the origin of the magnetic field in the central few hundred parsecs of the Galaxy. He also studies the hot, diffuse gas at the Galactic center with the Chandra X-ray observatory.
  • Michael Rich is a member of the Galaxy Evolution Explorer science team, a UV sky survey satellite. Rich's research on GALEX addresses the study of star formation in the 0

Postdoctoral Research

Graduate Student Research

  • Breann Sitarski works with Andrea Ghez on the kinematics and morphology of the Orion star-forming region in an effort to better understand the strong dynamical interactions that may be related to outflows around the stars. She is also interested in studying the properties of circumstellar disks.
  • Betsy Mills works with Mark Morris on data from an HST-NICMOS survey of the innermost 90 parsecs of the Galactic center in the Paschen alpha emission line. She is investigating the magnetic alignment of fine scale filamentary structure in the ionized gas in this region.
  • Kim Phifer works with Andrea Ghez to study the dynamics of the Milky Way nuclear stellar cluster using OSIRIS spectroscopy and NIR imaging obtained using Laser Guide Star Adaptive Optics with the Keck telescopes.
  • Sylvana Yelda works w/ Andrea Ghez using NIR images taken with the Keck II Laser Guide Star Adaptive Optics system to study the distribution of stars in the central parsec of our Galaxy. She is also interested in understanding the role of binaries in the origin of the young stars at the Galactic Center.

Select Publications:

Former Graduate Students and Postdocs

  • David Law studies the structure and dynamics of galaxies. Current research projects include using infrared IFU imaging and spectroscopy to determine the morphology and kinematics of galaxies at redshift z~ 2-3, and using N-body models of Local Group satellite galaxies to map out the mass distribution within the dark matter halo of the Milky Way.
  • Steve Berukoff works with Brad Hansen on understanding the stellar dynamics of the Galactic Center through numerical simulations.
  • Christian Howard works with Mark Morris and Mike Muno studying the diffuse X-ray plasma in the galactic center.
  • Joerg-Uwe Pott's research focusses on the application of new high angular resolution techniques to observe dusty stellar environments, phenomena in the Galactic center, and AGNs. He likes the challenges of interferometry from radio to optical wavelengths, and uses telescope arrays to resolve phenomena close to the central black holes in galaxies. Currently he is involved in the ASTRA-sensitivity upgrade of the Keck Interferometer as instrument scientist, and spends half of his time at the Keck telescopes.
  • Jessica Lu works with Andrea Ghez to understand recent star formation at the Galactic Center. She uses the Keck telescopes and the Laser Guide Star adaptive optics system to collect near-infrared images and spectra of the Galactic Center.
  • Jon Mauerhan works with Mark Morris and uses the Millimeter Interferometer Array at Owens Valley to study the 3-mm radio emission from the supermassive black hole at the Galactic Center. He also works with Mike Muno to search for infrared counterparts to X-ray binaries toward the Galactic Center
  • Dr. Andrea Stolte (postdoc) is a postdoctoral scholar working with Dr. Andrea Ghez on starburst clusters in the Milky Way. She studies the origin of the Arches cluster near the Galactic Center with Keck LGS-AO, and is interested in low-mass star formation and disk survival in NGC 3603 in the Carina arm.
  • Seth Hornstein worked with Andrea Ghez studying the variability of the infrared counterpart to the supermassive black hole at the Galactic Center. Seth is also involved in the dynamical motion study of the stellar cluster closest to the black hole.
  • Cornelia Lang (grad) worked with Mark Morris on high resolution mapping of the thermal and non-thermal filaments at the galactic center with the VLA.
  • Michael Muno (postdoc) is a Hubble fellow interested in the population of Galactic white dwarfs, neutron stars, and black holes. His current project is a multi-wavelength study of thousands of Chandra X-ray sources in the central 300 pc of our Galaxy. He has recently discovered that accreting black holes are highly concentrated within the central parsec of our Galaxy and may have settled there through dynamical friction.
  • Angelle Tanner (grad) worked with Andrea Ghez, Mark Morris and Eric Becklin on an unique collection of extended infrared sources located at the Galactic Center.


Last updated: Monday, 12-Aug-2013 16:32:00 PDT.
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