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telescopes (high-resolution spectroscopy) and space-based telescopes (asteroseismology). The uniting theme of these research projects is to expand our understanding of stars with masses similar to the Sun
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I supervise a wide range of projects in stellar astrophysics, with a focus on low and intermediate-mass stars, which have masses similar to or slightly larger than our Sun. This work is carried out
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regime, tidal disruption events, kilonovae and gamma ray burst afterglows. Some examples include: What do the spins of merging black holes tell us about binary evolution? Where are low-mass X-ray binaries
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constraints on the source properties(including neutron star mass and radius). Collaborative opportunities areavailable via project partners in the Netherlands, Denmark, and USA. The GOTO telescope networkwill
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stars and whether the potential planet signatures can be associated with the diversity of planetary properties (e.g. mass, radius, orbit, formation and dynamical history etc.). The main goal
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I work on the study of massive and supermassive stars (10-100,000 solar masses); the first generations of stars in the universe (Pop III stars); evolution of rotating massive stars and the spin