Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Univ. Aarhus
University of Victoria;
Univ. of Victoria;
Aarhus Univ
Aarhus University, Aarhus, Denmark
Department of Physics and Astronomy, University of Aarhus, Aarhus, Denmark;
Department of Physics and Astronomy, Aarhus University, Denmark
Aarhus Univ.
Dominion Astrophysical Observatory;
Aarhus;
Institute of Physics and Astronomy, Aarhus University, Ny Munkegade, 8000 Aarhus C, Denmark
U. Aarhus, Inst. of Physics and Astronomy
Department of Physics and Astronomy, University of Aarhus, bygn. 1520, Ny Munkegade, DK-8000 Aarhus C, Denmark
Institute of Physics and Astronomy, University of Århus, Ny Munkegade, DK-8000 Århus C, Denmark
Institute of Physics and Astronomy, Aarhus University, Ny Munkegade, 8000 Aarhus C, Denmark of Astronomy, University of Aarhus, Denmark
Department of Physics and Astronomy, Aarhus University, Ny Munkegade, 8000 Aarhus C, DK
Aahrus
Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Victoria, BC V8W 3P6, Canada; Guest user, Canadian Astronomy Data Centre, which is operated by the Dominion Astrophysical Observatory for the Canadian National Research Council's Herzberg Institute of Astrophysics; Institute of Physics and Astronomy, Aarhus University, Ny Munkegade, 8000 Aarhus C, Denmark of Physics and Astronomy, University of Aarhus, Denmark
Univ. of Aarhus
University of Victoria
Danish AsteroSeismology Centre, Department of Physics and Astronomy, University of Aarhus, DK-8000 Aarhus C, Denmark of Physics and Astronomy University of Aarhus DK-8000 Aarhus C, Denmark of Physics and Astronomy, University of Aarhus, Bygn. 520, 8000 Aarhus C, Denmark of Physics and Astronomy, University of Aarhus, DK--8000, Aarhus C, Denmark
Department of Physics and Astronomy, Aarhus University, Ny Munkegade, 8000 Århus C, Denmark Astrophysical Observatory, 5071 W. Saanich Road, Vic
A Distance-Independent Age for the Globular Cluster M92
A large C+N+O abundance spread in giant stars of the globular cluster NGC 1851
A multi-site campaign to measure solar-like oscillations in Procyon. I. Observations, Data Reduction and Slow Variations
A multi-site campaign to measure solar-like oscillations in Procyon. II. Mode frequencies
A new international project: Stellar Oscillations Network Group
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