The CoRoT target HD 49933 II. Comparison of theoretical mode amplitudes with observations

Astronomy and Astrophysics

Volumn 509, Issue 1, 2010, Pages

  Samadi, R ^a   Ludwig, H G ^b   Belkacem, K ^a,c   Goupil, M J ^b   Benomar, O ^d   Mosser, B ^a   Dupret, M A ^a,c   Baudin, F ^d   Appourchaux, T ^d   Michel, E ^a  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c UNIVERSITY OF LIÈGE   (Belgium)

^d UNIVERSITÉ PARIS SUD   (France)

Author keywords

Convection Turbulence Stars; HD 49933; Helioseismology Stars; Individual; Oscillations Sun

Indexed keywords

CAPILLARY FLOW; GEOPHYSICAL PROSPECTING; METALS; MIXTURES; SEISMIC RESPONSE; SEISMIC WAVES; STARS; STOCHASTIC SYSTEMS;

ADIABATIC APPROXIMATIONS; HD 49933; HELIOSEISMOLOGY; INDIVIDUAL; OSCILLATIONS-SUN; SOLAR LIKE OSCILLATIONS; STOCHASTIC EXCITATION MODELS; STOCHASTIC EXCITATIONS;

STOCHASTIC MODELS;

EID: 76349094474     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911868     Document Type: Article

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