Combining seismology and spectropolarimetry of hot stars

[en] Asteroseismology and spectropolarimetry have allowed us to progress significantly in our understanding of the physics of hot stars over the last decade. It is now possible to combine these two techniques to learn even more information about hot stars and constrain their models. While only a few magnetic pulsating hot stars are known as of today and have been studied with both seismology and spectropolarimetry, new opportunities - in particular Kepler2 and BRITE - are emerging and will allow us to rapidly obtain new combined results.

Disciplines :

Space science, astronomy & astrophysics

Author, co-author :

Neiner, Coralie

Briquet, Maryline ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie

Mathis, Stéphane

Degroote, Pieter

Language :

English

Title :

Combining seismology and spectropolarimetry of hot stars

Publication date :

2014

Event name :

IAU Symposium 307: New windows on massive stars: asteroseismology, interferometry and spectropolarimetry

Event date :

from 23-06-2014 to 27-06-2014

Audience :

International

Main work title :

IAU Symosium 307

Pages :

443

Additional URL :

http://adsabs.harvard.edu/abs/2014arXiv1407.8087N

Commentary :

proceedings of the IAU Symposium 307 held in Geneva in June 2014

Available on ORBi :

since 27 November 2014

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Bibliography

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