Frequency ratio method for seismic modelling of γ Doradus stars II. The role of rotation

Astronomy and Astrophysics

Volumn 443, Issue 1, 2005, Pages 271-282

  Suarez J C ^a,b   Moya, A ^b   Martin Ruiz S ^a   Amado, P J ^c   Grigahcene A ^a   Garrido, R ^a  

^a INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c EUROPEAN SOUTHERN OBSERVATORY   (Chile)

Author keywords

Stars: evolution; Stars: fundamental parameters; Stars: general; Stars: individual: HD 48501; Stars: oscillations; Stars: rotation

Indexed keywords

COMPUTATION THEORY; COMPUTER SIMULATION; ERROR ANALYSIS; GAMMA RAYS; PERTURBATION TECHNIQUES; ROBUSTNESS (CONTROL SYSTEMS);

STARS: EVOLUTION; STARS: FUNDAMENTAL PARAMETERS; STARS: GENERAL; STARS: INDIVIDUAL: HD 48501; STARS: OSCILLATIONS; STARS: ROTATION;

SEISMIC PROSPECTING;

EID: 27844545791     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20053114     Document Type: Article

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