CoRoT-2a magnetic activity: hints for possible star-planet interaction (2009)
Pagano, Isabella, Lanza, Antonino F., Leto, Giuseppe, Messina, Sergio, Barge, Pierre, Baglin, Annie
CoRoT-2a is a young (about 0.5 Gyr) G7V star accompanied by a transiting hot-Jupiter, discovered by the CoRoT satellite (Alonso et al. 2008; Bouchy et al. 2008). An analysis of its photospheric...
CoRoT Measures Solar-Like Oscillations and Granulation in Stars Hotter Than the Sun (2008)
Michel, Eric, Baglin, Annie, Auvergne, Michel, Catala, Claude, Samadi, Reza, Baudin, Frédéric, ...
4 pages, 3 figures.-- Supporting Online Material: Text, Fig. S1, Table S1 and References, available at: http://www.sciencemag.org/cgi/content/full/322/5901/558/DC1
CoRoT measures solar-like oscillations and granulation in stars hotter than the Sun (2008)
Michel, Eric, Baglin, Annie, Auvergne, Michel, Catala, Claude, Samadi, Reza, Baudin, Frédéric, ...
Jean Schneider, Michel Auvergne, Annie Baglin, Claude Catala, Magali Deleuil, Rafael Garrido, ...
COROT is a space mission approved by the French Space Agency CNES. Its goal is to make a significant step forward in the understandig of the origins and destiny of stars and of planetary systems. 1
Seismology and activity of the F type star HD 49933 (2005)
Mosser, Benoît, Bouchy, François, Catala, Claude, Michel, Eric, Samadi, Reza, Thévenin, Frédéric, ...
A 10-night asteroseismic observation programme has been conducted in January 2004 with the spectrometer Harps at the ES0 3.6-m telescope. The selected target, the 6th magnitude F5V star HD 49933, was...
Seismology and activity of the F type star HD 49933 (2005)
Mosser, Benoît, Bouchy, François, Catala, Claude, Michel, Eric, Samadi, Reza, Thévenin, Frédéric, ...
A 10-night asteroseismic observation programme has been conducted in January 2004 with the spectrometer Harps at the ES0 3.6-m telescope. The selected target, the 6th magnitude F5V star HD 49933, was...
Seismology and activity of the F type star HD 49933 (2005)
Mosser, Benoît, Bouchy, François, Catala, Claude, Michel, Eric, Samadi, Reza, Thévenin, Frédéric, ...
A 10-night asteroseismic observation programme has been conducted in January 2004 with the spectrometer Harps at the ES0 3.6-m telescope. The selected target, the 6th magnitude F5V star HD 49933, was...
Seismology and activity of the F type star HD 49933 (2005)
Mosser, Benoît, Bouchy, François, Catala, Claude, Michel, Eric, Samadi, Reza, Thévenin, Frédéric, ...
A 10-night asteroseismic observation programme has been conducted in January 2004 with the spectrometer Harps at the ES0 3.6-m telescope. The selected target, the 6th magnitude F5V star HD 49933, was...
Seismology and activity of the F type star HD 49933 (2005)
Mosser, Benoît, Bouchy, François, Catala, Claude, Michel, Eric, Samadi, Reza, Thévenin, Frédéric, ...
A 10-night asteroseismic observation programme has been conducted in January 2004 with the spectrometer Harps at the ES0 3.6-m telescope. The selected target, the 6th magnitude F5V star HD 49933, was...
Seismology and activity of the F type star HD 49933 (2005)
Mosser, Benoît, Bouchy, François, Catala, Claude, Michel, Eric, Samadi, Reza, Thévenin, Frédéric, ...
A 10-night asteroseismic observation programme has been conducted in January 2004 with the spectrometer Harps at the ES0 3.6-m telescope. The selected target, the 6th magnitude F5V star HD 49933, was...
Oscillation power across the HR diagram : sensitivity to the convection treatment (2001)
Samadi, Reza, Houdek, Guenter, Goupil, Marie-Jo, Lebreton, Yveline, Baglin, Annie
Solar-like oscillations are stochastically excited by turbulent convection. In this work we investigate changes in the acoustic oscillation power spectrum of solar-type stars by varying the treatment...
Comparative seismology of pre- and main sequence stars in the instability strip (2001)
Suran, Marian, Goupil, MarieJo, Baglin, Annie, Lebreton, Yveline, Catala, Claude
Pulsational properties of 1.8 M$_{\odot}$ stellar models covering the latest stages of contraction toward the main sequence up to early hydrogen burning phases are investigated by means of linear...
Oscillation power as a test of stellar turbulence : Scanning the HR diagram (2001)
Samadi, Reza, Goupil, Marie-Jo, Lebreton, Yveline, Baglin, Annie
The acoustic power injected by turbulent convection into solar-like oscillations depends on the details of the turbulent spectrum. A theoretical formulation for the oscillation power is developed...
De l'évolution des étoiles dégénérées chaudes / (1967)
Thesis (doctoral)--Université de Paris, 1967.
Propagation des ondes dans un milieu partiellement ionisé (1961)
On étudie la propagation des ondes de basse fréquence et leur amortissement dans un milieu partiellement ionisé, indéfini, uniforme, plongé dans un champ magnétique Bo. On étudie uniquement le...
Propagation des ondes dans un milieu partiellement ionisé (1961)
On étudie la propagation des ondes de basse fréquence et leur amortissement dans un milieu partiellement ionisé, indéfini, uniforme, plongé dans un champ magnétique Bo. On étudie uniquement le...
Propagation des ondes dans un milieu partiellement ionisé (1961)
On étudie la propagation des ondes de basse fréquence et leur amortissement dans un milieu partiellement ionisé, indéfini, uniforme, plongé dans un champ magnétique Bo. On étudie uniquement le...