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Duncan Galloway's primary research interest lies in the nature and properties of neutron star binaries, particularly focusing on supernova explosions and the extreme conditions of surface density, temperature, and magnetic field strength. His work involves observational studies using satellite-based X-ray observatories to gather insights on accreting binaries and their unique physical characteristics. Duncan studied at the University of Tasmania where he completed his undergraduate degree before working for five years as an oceanographer. He later transitioned to astrophysics, holding several postdoctoral positions at prestigious institutions, including the Massachusetts Institute of Technology. His research spans various topics, including accretion-powered millisecond pulsars and thermonuclear X-ray bursts, employing advanced X-ray observatories from NASA and the European Space Agency. He is a principal investigator on the Gravitational-wave Optical Transient Observatory (GOTO) project, aiming to enhance the understanding of gravitational wave sources through optical and X-ray observations. Duncan’s contributions are noteworthy in the field of astrophysics, particularly regarding the physical processes governing neutron stars and their equation of state.
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