Today’s authors look at how the frequency of stellar flares evolves for different types of star.
Today’s authors have possibly found a new type of variable star in a class of massive supergiant stars.
The structure of oscillations in intermediate mass stars has eluded astronomers, until now.
Today’s authors use asteroseismology to glance inside stars with long-period variability.
How can we make academic posters clear, concise, and quick without sacrificing information?