Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Astronomy Department, Ohio State University
OSU
University College, London, England
Ohio State University
Joint Institute for Laboratory Astrophysics, Boulder, Colo.
Joint Institute for Laboratory Astrophysics, Boulder, CO
Windsor, University, Windsor, Ontario, Canada
Dept of Astronomy, and ChemicalPhysics Program, The OhioState University, Columbus, OH 43210
The Queen's University of Belfast, Belfast, Northern Ireland, UK
Ohio State University, Columbus, Ohio, US
Department of Astronomy, The Ohio State University, 174 West 18th Avenue, Columbus, OH 43210-1106, USA of Astronomy, The Ohio State University, Columbus, OH 43210, USA of Astronomy, The Ohio State University, USA
The Ohio State University
Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA of Astronomy, The Ohio State University, Columbus, OH 43210, USA
Department of Astronomy, The Ohio State University, Columbus, OH 43210, USA of Astronomy, Ohio State University, 174 West 18th Avenue, Columbus, OH 43210-1106, USA
Ohio State University, Columbus
Ohio State University, Columbus, OH, US
Department of Astronomy, Ohio State University, 140 West 18th Avenue, Columbus, OH 43210-1106, USA
Joint Institute for Laboratory Astrophysics, University of Colorado and National Bureau of Standards, Boulder, CO 80309-0440
Department of Astronomy, Ohio State University, 174 West 18th Avenue, Columbus, OH 43210-1106
Department Astronomy, Ohio State University
Ohio State
Department of Astronomy, The Ohio State University - USA
Dept. Astronomy, Ohio State Univ
Department of Astronomy, The Ohio State University, Columbus, Ohio, USA
Dept. of Astronomy, The Ohio State University
Dept. of Astronomy, Ohio State
Ohio State, USA
Department of Astronomy, The Ohio State University
(Fe II) emission from high-density regions in the Orion Nebula
A Near-Infrared Template Derived from I Zw 1 for the FeII Emission in Active Galaxies
A remarkable long-term light curve, and deep, low-state spectroscopy: Swift & XMM-Newton monitoring of the NLS1 galaxy Mkn 335
A study of the breakdown of the quasi-static approximation at high densities and its effect on the helium-like K ALPHA complex of nickel, iron, and calcium
Accuracy of Stellar Opacities and the Solar Abundance Problem
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