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stars, students, and alumni and support Monash wide initiatives such as the STEMM women academic network and champion accessibility , and much more. We provide staff with carer travel support and
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: Visualisation of a plan generated by SCIPPlan for an example navigation domain where the red square represents the agent, the blue rectangles represent the blocks, the gold star represents the goal location and
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Observatory (LIGO) in order to understand the fate of massive stars, to probe how binary black holes form, and to understand the nature of matter at the most extreme possible densities. Occasionally, we
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I offer projects broadly related to supernova explosions and the final stages in the lives of massive stars. Specific topics of interest include fluid dynamics processes in stellar explosions and
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the evolution of massive binary stars into compact binaries as sources of gravitational-waves and astrophysical inference on gravitational-wave observations. My research group on massive binary evolution -- also
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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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My research interests focus on the stars - primarily their structure, evolution and nucleosynthesis. This can involve modelling of mixing in stars, or effects of changing nuclear burning rates
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I am interested in the most catastrophic and explosive collisions in the Universe, such as the mergers of neutron stars and black holes. I study these using both gravitational waves and
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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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My primary areas of research activity are twofold:first, studing thermonuclear (X-ray) bursts from accreting neutron stars;and second, searches for optical counterparts of gravitational-wave