Betelgeuse's recent dimming event is just one of many intriguing phenomena displayed by this exquisite exemplar of red supergiants. In this invited review I will discuss what is known and thought about variability of red supergiants. This will focus on variations on dynamical and thermal timescales, such as convection, pulsation, and possible eruptions shortly before core collapse or mantle depletion; as well as hydrodynamic, electro-magnetic, and chemo-thermal instabilities from the photosphere out through the wind. The aim is to arrive at a holistic picture of how and why red supergiants vary and shed mass, making their own contribution to the entropy increase of the Univers
Context. It has been proposed that convection in red supergiant (RSG) stars produces large-scale g...
Aims. This research has two main goals. First, we present the atmospheric structure and the fundamen...
Red supergiants are a class of massive stars, who will soon end their lives as supernovae. Time vari...
Red giants and red supergiants have long been known to be variable. In the last 40 years many of the...
Context.Red supergiant stars represent a key phase in the evolution of massive stars. Recent radia...
Betelgeuse is a pulsating red supergiant whose brightness is semi periodically variable and in Febru...
Context: Red supergiant stars represent a key phase in the evolution of massive stars. Recent radiat...
Red supergiants are the most common final evolutionary stage of stars that have initial masses betwe...
Context. Red supergiant (RSGs) are cool massive stars in a late phase of their evolution when the st...
International audienceABSTRACT The rate at which mass is lost during the red supergiant (RSG) evolut...
We study the brightness variations of galactic red supergiant stars using long-term visual light cur...
Attention is given to the theoretical period-luminosity-color relations of stars evolving with mass ...
We review the significant role played by red supergiants (RSGs) in stellar populations, an...
Context. Red supergiants are observed to undergo vigorous mass loss. However, to date, no theoretica...
Context. Red supergiant (RSGs) are cool massive stars in a late phase of their evolution when the st...
Context. It has been proposed that convection in red supergiant (RSG) stars produces large-scale g...
Aims. This research has two main goals. First, we present the atmospheric structure and the fundamen...
Red supergiants are a class of massive stars, who will soon end their lives as supernovae. Time vari...
Red giants and red supergiants have long been known to be variable. In the last 40 years many of the...
Context.Red supergiant stars represent a key phase in the evolution of massive stars. Recent radia...
Betelgeuse is a pulsating red supergiant whose brightness is semi periodically variable and in Febru...
Context: Red supergiant stars represent a key phase in the evolution of massive stars. Recent radiat...
Red supergiants are the most common final evolutionary stage of stars that have initial masses betwe...
Context. Red supergiant (RSGs) are cool massive stars in a late phase of their evolution when the st...
International audienceABSTRACT The rate at which mass is lost during the red supergiant (RSG) evolut...
We study the brightness variations of galactic red supergiant stars using long-term visual light cur...
Attention is given to the theoretical period-luminosity-color relations of stars evolving with mass ...
We review the significant role played by red supergiants (RSGs) in stellar populations, an...
Context. Red supergiants are observed to undergo vigorous mass loss. However, to date, no theoretica...
Context. Red supergiant (RSGs) are cool massive stars in a late phase of their evolution when the st...
Context. It has been proposed that convection in red supergiant (RSG) stars produces large-scale g...
Aims. This research has two main goals. First, we present the atmospheric structure and the fundamen...
Red supergiants are a class of massive stars, who will soon end their lives as supernovae. Time vari...