Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
University of Chicago
Department of Chemistry and Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois
Department of Physics, Toyama University, Gofuku, Toyama 930, Japan
Chicago University
Department of Astronomy & Astrophysics and Department of Chemistry, University of Chicago, Chicago, IL 60637
Department of Astronomy and Astrophysics, Department of Chemistry, and The Enrico Fermi Institute, University of Chicago, Chicago, IL 60637
Department of Chemistry and Department of Astronomy and Astrophysics, The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637
Departments of Chemistry, Astronomy & Astrophysics, University of Chicago
Department of Chemistry, The University of Chicago, Chicago, Illinois 60637-1403 USA
Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637
Chicago Univ., IL
Department of Astronomy and Astrophysics, and Department of Chemistry, the University of Chicago, IL 60637
Department of Astronomy and Astrophysics, and Department of Chemistry, The Enrico Fermi Institute, the University of Chicago, IL 60637
Department of Astronomy and Astrophysics and Department of Chemistry, University of Chicago, Chicago, IL 60637
Department of Chemistry, Department of Astronomy & Astrophysics, and the Enrico Fermi Institute, University of Chicago, Chicago, IL 60637
Department of Astronomy and Astrophysics and Department of Chemistry, The Enrico Fermi Institute, University of Chicago, Chicago, IL 60637
Chicago, University, IL
Department of Chemistry and Department of Astronomy and Astrophysics, The University of Chicago, Chicago, Illinois 60637
Department of Chemistry, The University of Chicago, Chicago, Illinois 60637 USA
A New Atlas of the Diffuse Interstellar Bands: HD 183143
A Search for H3+ in Planetary Nebulae and Proto-planetary Nebulae
A table of astronomically important ro-vibrational transitions for the H3(+) molecular ion
Absorption Line Survey of H3+ toward the Galactic Center Sources II. Eight Infrared Sources within 30 pc of the Galactic Center
Comparing the Ortho-To Ratios of H_2 and H_3^+ in Diffuse Interstellar Clouds
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