Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
Astronomy Dept., University of Texas
University of Texas, Austin
University of Texas at Austin
Abundances In Very Metal Poor Dwarf Stars
Chemical Evolution of the Halo and Disk of the Galaxy
Chemical Evolution of the Halo and Disk of the Galaxy
Circumstellar Material in Type Ia Supernovae via Sodium Absorption Features
Metal Abundances and Mixing in Metal-Rich Globular Clusters with Blue Horizontal Branches
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