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to uncover how mass loss depends on stellar properties such as pulsation, luminosity, temperature, and mass Position B: Binary Star Evolution with Gaia This position focuses on understanding how interactions
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secure interaction between converters and the surrounding network has therefore emerged as one of the most challenging topics in modern power systems research. We seek an exceptional postdoctoral
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in observed binaries. An observation-driven modelling approach is envisioned, with the aim to calibrate tidal dissipation in binary evolution models of interacting dynamical rotating stars. Applicants
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