Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
Dublin
Dublin Institute for Advanced Studies, Dublin, Ireland
external author
School of Cosmic Physics, Dublin Inst. for Advanced Studies, 5 Merrion Square, Dublin 2, Ireland
Dublin Institute for Advanced Studies, Republic of Ireland
Max-Planck-Institut für Kernphysik, Heidelberg, Germany
Dublin Institute for Advanced Studies, 5 Merrion Square, Dublin 2, Ireland
Dublin Institute for Advanced Studies, IRL-Dublin 2, Ireland
Dublin Inst. for Advanced Studies, Dublin, Ireland
Dublin Institute for Advanced Studies School of Cosmic Physics
Dublin Inst. for Advanced Studies, Ireland
School of Cosmic Physics, Dublin Institute for Advanced Studies
Dublin Institute for Advanced Studies, Ireland
Max-Planck-Inst. für Kernphysik, Heidelberg, Germany
Max-Planck-Inst. für Kernphysik
National Center for Atmospheric Research
Wien University
Cambridge University, Cambridge, England
School of Cosmic Physics, Dublin Institute for Advanced Studies, 5 Merrion Square, Dublin 2, Ireland
Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland
Dublin Institute for Advanced Studies, School of Cosmic Physics, 5Merrion Square, Dublin2, Ireland
Dublin Institute for Advanced Studies, School of Cosmic Physics, 5 Merrion Square, Dublin2, Ireland
Dublin Institute for Advanced Studies
Dublin Institute for Advanced Studies, 5 Merrion Square, Dublin 2, Republic of Ireland
Dublin Institute for Advanced Studies, School of Cosmic Physics, Astronomy and Astrophysics Section, 31 Fitzwilliam Place, Dublin 2, Ireland
Dublin Institute for Advanced Studies Dublin 2, Ireland
Dublin Institute for Adv
22nd International Cosmic Ray Conference. Proceedings.
A comparison of models for supernova remnants including cosmic rays
A Constraint on Prompt Supernova Cosmic-Ray Production from Gamma-Ray Observations
A cosmic ray driven instability
A Cosmic-ray Composition Controlled by Volatility and a/q Ratio. SNR Shock Acceleration of gas and Dust
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