Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
ESA, Noordwijk, The Netherlands
Physics Department, University of Birmingham, UK
Observatoire de la Côte d'Azur
Nice Obs.
Universite Paris, Orsay, France
Space Science Department of ESA, Noordwijk, Netherlands
Physikalisch-Meteorologisches Observatorium, Davos, Switzerland
School of Physics and Astronomy, University of Birmingham, Birmingham, UK of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK
Observatoire de Nice, B.P. 4229, F-06304 Nice Cedex 4, France
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK; Institute of Theoretical Astrophysics, University of Oslo, PO Box 1029 Blindern, 0315 Oslo, Norway tierry.
Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029, Blindern, N-0315 Oslo, Norway
ESTEC, Noordwijk, Netherlands
Département Cassini, URA CNRS 1362, Observatoire de la Côte d'Azur, F-06304 Nice, France; and Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029, N-0315 Oslo, Norway.
Département Cassini, URA CNRS 1362, Observatoire de la Côte d'Azur, 06304 Nice, France; Institute of Theoretical Astrophysics, University of Oslo, PO Box 1029, 0315 Oslo, Norway
Département Cassini, UMR CNRS 6529, Observatoire de la Côte d'Azur, F-06304 Nice, France
Institut d'Astrophysique, Paris, France
Centre National de la Recherche Scientifique, Verrieres-Le Buisson, France
Space Science Department of ESA, Noordwijk, The Netherlands
Département Cassini, UMR CNRS 6529, OCA, BP 4229, 06304 Nice cedex 04, France
Departement Cassini, URA CNRS 1362, Observatoire de la Cote d' Azur
A framework for describing correlated excitation of solar p modes
A fresh look at the seismic spectrum of HD49933: analysis of 180 days of CoRoT photometry
A new estimate of the solar core rotation from IPHIR
About structure inversions of simulated COROT data for a solar like star
An Eulerian approach for the computation of oscillation mode visibility
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