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The project SUPERSTARS-3D aims to develop the first three-dimensional models of atmospheres for hot, massive stars. This advancement will enhance our understanding of these stars and improve the analysis of their radiation, which is crucial for studying cosmic phenomena like black holes and gravitational waves.
Stars with masses many times that of our Sun are the direct progenitors to cosmic phenomena such as supernova explosions, black holes, and gravitational wave (GW) sources.
Through electromagnetic observations we obtain empirical information of such massive stars, however decoding the radiation reaching us through our telescopes is a highly non-trivial exercise.
To constrain fundamental properties like temperatures, radii, chemical abundances, and mass loss, the observed radiation is fit by means…
KATHOLIEKE UNIVERSITEIT LEUVEN
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