Add to ORKGAbstract. A review of the ability of asteroseismology to probe the internal physics of OB stars is presented. The main constraints that can be obtained from the frequency spectrum in p-and g-modes pulsators are discussed. Next, we consider energetic aspects of the pulsations in OB stars and show how such study also allows to constrain their internal physics. The cases of p-mixed modes (β Cep stars), g-modes (SPB stars), strange modes and stochastically excited modes are considered
Hot subdwarf stars, including helium core burning subdwarf B (sdB) stars and more evolved subdwarf O...
Asteroseismology provides us with a unique opportunity to improve our understanding of stellar struc...
Asteroseismology probes the internal structures of stars by using their natural pulsation frequencie...
A review of the ability of asteroseismology to probe the internal physics of OB stars is presented. ...
Recent space observations with CoRoT and ground-based spectroscopy have shown the presence of differ...
After a brief introduction into the asteroseismic modelling of stars, we provide a compilation of th...
The recent research domain of asteroseismology studies the internal structure of stars, which is not...
The region of the hot end of the main-sequence is hosting pulsating stars of different types and fla...
Context. The β Cephei pulsators are massive, ∼8−25 M⊙ essentially on the main sequence, stars. The n...
Context. Very high precision seismic space missions such as CoRoT and Kepler provide the means for t...
Context. Asteroseismology of Sun-like stars is undergoing rapid expansion with, for example, new dat...
Context. Very high precision seismic space missions such as CoRoT and Kepler provide the means for t...
Hot subdwarf stars (of the sdB and sdO type) host three known classes of nonradial pulsators. Two of...
We present new methodological developments regarding the treatment of the asteroseismic surface term...
Asteroseismology is a recent branch of astrophysics that studies the interiors of stars by the inter...
Hot subdwarf stars, including helium core burning subdwarf B (sdB) stars and more evolved subdwarf O...
Asteroseismology provides us with a unique opportunity to improve our understanding of stellar struc...
Asteroseismology probes the internal structures of stars by using their natural pulsation frequencie...
A review of the ability of asteroseismology to probe the internal physics of OB stars is presented. ...
Recent space observations with CoRoT and ground-based spectroscopy have shown the presence of differ...
After a brief introduction into the asteroseismic modelling of stars, we provide a compilation of th...
The recent research domain of asteroseismology studies the internal structure of stars, which is not...
The region of the hot end of the main-sequence is hosting pulsating stars of different types and fla...
Context. The β Cephei pulsators are massive, ∼8−25 M⊙ essentially on the main sequence, stars. The n...
Context. Very high precision seismic space missions such as CoRoT and Kepler provide the means for t...
Context. Asteroseismology of Sun-like stars is undergoing rapid expansion with, for example, new dat...
Context. Very high precision seismic space missions such as CoRoT and Kepler provide the means for t...
Hot subdwarf stars (of the sdB and sdO type) host three known classes of nonradial pulsators. Two of...
We present new methodological developments regarding the treatment of the asteroseismic surface term...
Asteroseismology is a recent branch of astrophysics that studies the interiors of stars by the inter...
Hot subdwarf stars, including helium core burning subdwarf B (sdB) stars and more evolved subdwarf O...
Asteroseismology provides us with a unique opportunity to improve our understanding of stellar struc...
Asteroseismology probes the internal structures of stars by using their natural pulsation frequencie...