Minimum 2:1 degree in physics or a related subject (or equivalent)
Months of entry
The majority of stars reside in binaries or higher multiples, and the most exotic and the most energetic phenomena in the Universe often have a binary origin. Binary stars are the keystones of stellar astrophysics, offering the chance to directly measure physical parameters of stars and so understand the evolution of the contents of the Universe. Within the Astronomy Discipline of the School of Physical Sciences, we carry out research on populations of binary stars, on specific classes of binary, and on individual systems. We have strengths in both multi-wavelength observational programmes as well as in theoretical and computer modelling studies. Around half a dozen postgraduate students currently pursue projects in this area, supported by four academic supervisors.
Potential research projects
We welcome enquiries from prospective students in the following areas:
- Variability in the SuperWASP stellar population
- Multiwavelength observations of interacting compact binary stars
- Evolution of compact binaries
- Synthetic stellar and binary populations.
Projects currently on offer may be found here.
Recent research projects include
- Unveiling the nature of magnetic cataclysmic variables
- The identification and classification of variability in SuperWASP stars
- A stellar variability survey with STEREO
- SuperWASP variable stars with varying periods
- Neutron star mass determinations and evolution of high mass X-ray binaries
- Evolutionary history of post-common envelope binaries
- Binary stars as false positives in exoplanet transit searches
Fees and funding
Qualification and course duration
Course contact details
- Administrative support
- +44 (0)1908 659036