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Dr. Ekaterina M Verner


Astrophysics Science Division
NASA/GSFC
Code 667, ExoPlanets & Stellar Astrophysics
Greenbelt, MD 20771

tel: 301-286-3019
fax:
e-mail: Ekaterina.M.Verner @ nasa.gov


Present Position

Adjunct Research Professor at Catholic University of America

Brief Bio

Dr. Verner did her M.Sc. at MGPI (RUSSIA) and Ph.D. at UofT(CANADA). She was at Goddard since 2001 after completining Ph D. Scientific interests include spectroscopy, line formation, elemental abundances studies in QSOs. She is a PI and co-I on several NASA and NSF grants to study topics related to Fe II spectra formation and line analysis in astrophysical plasma.

Educational Background

Ph. D. in Astrophysics, Univ. of Toronto, Canada, Jun. 2000
Thesis Advisor: Prof. Peter Martin, Thesis Title: “Fe II Emission from H II Regions and Active Galactic Nuclei”
M. S. in teaching of physics and astronomy, Moscow State Pedagogical Institute (MGPI), 1984
Special education in math and physics, physics and mathematics school N2, Moscow, 1979

Research Interests

Theoretical and observational studies of chemical abundances and physical conditions in interstellar medium, nebulae, symbiotics, and quasars - Photoionization modeling of astrophysical plasmas - Atomic data for astrophysics - Excitation mechanisms of molecules in comets - Chemical equilibrium modeling for molecules in envelopes of carbon rich stars

Current Projects

NSF, theoretical studies, "Tracing the Metallicity in High Redshift Quasars with Fe II Spectra, Grant AST-0206150, E. Verner (PI)

NASA, SPITZER observations, "Spitzer Imagery & Spectroscopy of Symbiotics with Extended Nebulosity", F. Bruhweiler (PI)

NASA, Eta Carinae spectroscopical studies, T. Gull (PI)

WRRI, “Air-deposited pollutants in the Anacostia river watershed”, A. Adebyao (PI)