CORDIS Project
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The project investigates the internal structures and physical conditions of red-giant stars using asteroseismology. By analyzing mixed dipole oscillation modes, it aims to uncover the differences in stellar structures and their evolution, enhancing our understanding of stars and their role in the universe.
What would a star look like below its opaque surface?
What are the physical conditions in a star?
What physical processes play an important role in stars?
How do these physical conditions and processes interact?
How do they change with time, when a star evolves?
Answering these kinds of questions is of fundamental importance for astronomy and beyond.
Stars are a dominant source of light in the universe as well as main building blocks of planetary systems and galaxies.
Thus, understanding of sta…
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