Department of Physics & Astronomy

Frederick Hamann

Fred Hamann

Frederick Hamann


Physics 3013/Pierce 2134B

Telephone: 951-827-5072
Email: frederick.hamann@ucr.edu
Fax: 951-827-4529


Research Interests:

  • Astrophysics. Quasars and active galaxies. Super-massive black holes in galactic nuclei. The formation and evolution of galaxies. Accretion and outflow processes in stars and galactic black hole environments. The high redshift universe. Galactic chemical enrichment. Early and late stages of stellar evolution. Spectroscopy with astrophysical applications. 


B.S. in Astronomy-Physics, B.S. in Mathematics - University of Wisconsin, 1981

Ph.D. in Astronomy - State University of New York at Stony Brook, 1987

Previous Employment:

Postdoctoral Fellow - Carnegie Observatories, Pasadena

Columbus Postdoctoral Fellow - The Ohio State University

Research Scientist - University of California, San Diego

Professor - University of Florida

Current Research:

I am currently leading research programs in three broad areas of astrophysics. One is the discovery and analysis of obscured/red quasars to understand their relationships to the early stages of quasar/galaxy evolution. Another focuses on quasar accretion disk outflows to understand the origins, energetics and physical properties of these flows and test their viability as a feedback mechanism that could regulate star formation and mass assembly in the host galaxies. A third employs quasar absorption lines to measure the full range of gaseous environments around quasars and derive further constraints on nature and evolutionary status of quasars in their host galaxies. The absorption line environments include quasar-driven outflows, ambient gas in galactic halos, remnants from recent messy mergers, starburst-driven blowouts that might accompanying quasar activity, and infall (“cold mode accretion”) from the inter-galactic medium that could be critical for galaxy assembly. These studies use numerical simulations and data from major observatories including the Hubble Space Telescope, the Chandra X-ray Observatory, the Atacama Large Millimeter (and sub-millimeter) Array, large ground-based facilities such as Keck, Gemini and the VLT, and wide-field surveys like the Sloan Digital Sky Survey (SDSS) and the Wide-field Infrared Survey Explorer (WISE). 

Recent Publications:

Full Publications List

More Information

General Campus Information

University of California, Riverside
900 University Ave.
Riverside, CA 92521
Tel: (951) 827-1012

Career OpportunitiesUCR Libraries
Campus StatusDirections to UCR

Department Information

Physics & Astronomy
Physics Building

Main Office Tel: (951) 827-5331
Main Office Fax: (951) 827-4529
Maynard, Bonnie; Chair's Assistant, Academic Personnel
E-mail: bonnie.maynard@ucr.edu