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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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-dependent process to a device-assisted platform by integrating zero-net-mass-flux synthetic jets, piezoelectric actuation and quantitative aerosol diagnostics into an adaptive soft-mist inhaler. Funded
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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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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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, Distance Less than 40 Mpc, SAGUARO, and Global Supernova Project. Here are a few examples of students' projects that can be adapted to suit the interests of students. Constraining the mass loss rate of red
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to provide constraints on the source properties (including neutron star mass and radius). Collaborative opportunities are available via project partners in the Netherlands, Denmark, and USA. The GOTO telescope
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distribution functions. Total content of H2 in the solar neighbourhood and nearby galaxies and how they compare to other gas/dust tracers. Extinction mapping from resolved stars in nearby galaxies. Studying mass
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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