Reference : Time-dependent convection seismic study of five gamma Doradus stars
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/75423
Time-dependent convection seismic study of five gamma Doradus stars
English
Dupret, Marc-Antoine [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique >]
Grigahcène, A. [Instituto de Astrofísica de Andalucía-CSIC, Apartado 3004, 18080 Granada, Spain; CRAAG - Algiers Observatory BP 63 Bouzareah 16340, Algiers, Algeria]
Garrido, R. [Instituto de Astrofísica de Andalucía-CSIC, Apartado 3004, 18080 Granada, Spain]
De Ridder, J. [Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200 B, 3001 Leuven, Belgium]
Scuflaire, Richard [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Evol. et stabilité des étoiles et des amas d'étoiles (ESEA) >]
Gabriel, Maurice [> > Département d'astrophys., géophysique et océanographie (AGO) >]
1-Jul-2005
Monthly Notices of the Royal Astronomical Society
Blackwell Publishing
360
1143-1152
Yes (verified by ORBi)
International
0035-8711
Oxford
United Kingdom
[en] convection ; stars: interiors ; stars: oscillations ; stars: variables: other
[en] We apply for the first time the time-dependent convection (TDC) treatment of Gabriel and Grigahcène et al. to the photometric mode identification in gamma Doradus (gamma Dor) stars. We consider the influence of this treatment on the theoretical amplitude ratios and phase differences. Comparison with the observed amplitudes and phases of the stars gamma Dor, 9 Aurigae, HD 207223 = HR 8330, HD 12901 and 48501 is presented and enables us to identify the degree l of the pulsation modes for four of them. We also determine the mode stability for different models of these stars. We show that our TDC models agree better with observations than with frozen convection models. Finally, we compare the results obtained with different values of the mixing-length parameter alpha.
http://hdl.handle.net/2268/75423
10.1111/j.1365-2966.2005.09114.x
http://adsabs.harvard.edu/abs/2005MNRAS.360.1143D

File(s) associated to this reference

Fulltext file(s):

FileCommentaryVersionSizeAccess
Restricted access
Dupret-gadophot2005.pdfPublisher postprint378.34 kBRequest copy

Bookmark and Share SFX Query

All documents in ORBi are protected by a user license.