- Home
- Volume 88 - Année 2019
- Actes de colloques
- How Much to we Trust Stellar Models ? - September ...
- Fast rotation and acoustic modes
since 05 February 2011 :
View(s): 520 (13 ULiège)
Download(s): 44 (0 ULiège)
View(s): 520 (13 ULiège)
Download(s): 44 (0 ULiège)
Daniel Roy Reese
Fast rotation and acoustic modes
(Volume 88 - Année 2019 — Actes de colloques — How Much to we Trust Stellar Models ? - September 2018 - Liège, Belgium)
Article
Attached document(s)
original pdf file Mots-clés : pulsations stellaires, rotation stellaire, structure stellaire, évolution stellaire
Abstract
In this contribution, we describe recent progress in modelling acoustic pulsations of rapidly rotating stars. We then go on to describe very recent attempts at interpreting pulsation spectra in two observed stars. These make use of multi-colour mode visibilities, mode excitation, and pulsation frequencies in order to con-strain the identification of the observed modes.
Keywords : stellar pulsations, stellar rotation, stellar structure and evolution
To cite this article
Daniel Roy Reese, «Fast rotation and acoustic modes», Bulletin de la Société Royale des Sciences de Liège [En ligne], Volume 88 - Année 2019, Actes de colloques, How Much to we Trust Stellar Models ? - September 2018 - Liège, Belgium, 106 - 114 URL : https://popups.uliege.be/0037-9565/index.php?id=9276.
About: Daniel Roy Reese
LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Univ. Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, 92195 Meudon, France