Reference : 2D non-perturbative modeling of oscillations in rapidly rotating stars
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/140134
2D non-perturbative modeling of oscillations in rapidly rotating stars
English
Ouazzani, Rhita-Maria mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie >]
Dupret, Marc-Antoine mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie >]
Goupil, M. J. [> >]
Reese, Daniel mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie >]
1-Jan-2010
Astronomical Notes
331
45
No
International
[en] Astrophysics - Solar and Stellar Astrophysics
[en] We present and discuss results of a recently developped two dimensional non-perturbative method to compute accurate adiabatic oscillation modes of rapidly rotating stars . The 2D calculations fully take into account the centrifugal distorsion of the star while the non-perturbative method includes the full influence of the Coriolis acceleration. These characteristics allows us to compute oscillation modes of rapid rotators - from high order p-modes in $\delta$Scuti stars, to low order p- and g-modes in $\beta$ Cephei or Be stars.
http://hdl.handle.net/2268/140134
http://adsabs.harvard.edu/abs/2013arXiv1301.2499O
4 pages, 1 figure, proceedings of the 4th HELAS International Conference, Lanzarote feb 2010, Astronomical Notes, 2010, 331, P 45

File(s) associated to this reference

Fulltext file(s):

FileCommentaryVersionSizeAccess
Restricted access
Ouazzani1.pdfPublisher postprint147.59 kBRequest copy

Bookmark and Share SFX Query

All documents in ORBi are protected by a user license.