Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
Washington University, St. Louis, MO 63130, USA
Co/Ni Ratio in Galactic Cosmic Rays: Results from the TIGER-2001 Flight
Cosmic-ray origin in OB associations and preferential acceleration of refractory elements: Evidence from abundances of elements 26Fe through 34Se
Elemental Abundances in the Cosmic Rays 26<=Z<=34 -- Evidence For Cosmic-Ray Origin in OB Associations
Elemental Abundances in the Galactic Cosmic Rays with Atomic Number (Z) in the Interval 30 to 40
Erratum: "Cosmic Ray Origin in OB Associations and Preferential Acceleration of Refractory Elements: Evidence from Abundances of Elements 26Fe Through 34Se" (2009, ApJ, 697, 2083)
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