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Multi-component angle/action based distribution function (DF) models can be optimised based on how well they reproduce observations thus revealing the…
Many stars, including our own Sun, pulsate in a great number of distinct and observable oscillation modes simultaneously. Tracing the deep stellar…
High resolution transmission spectroscopy is one of the main techniques for exoplanet atmosphere characterisation. Planetary absorption can be…
Stars are self-gravitating fluids in which many types of waves can propagate. Constructive interference of these waves produces global modes of…
Chemical abundances in stars and gas tell us about the formation and evolution of galaxies, as well as stellar nucleosynthesis. I will discuss how we…
The Carrington storm in 1859 is considered one of the earliest and largest magnetic storms during magnetic observations covering 180 years. While some…
Stellar physics has many applications and here I present a number of examples related to formation of planets, supernovae, X-ray binaries as well as…