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Research degrees
Research areas
Astronomy
Stellar astrophysics

Stellar astrophysics

Qualifications Duration Start dates Application period
PhD
(MPhil also available)
Full-time: 3–4 years
Part-time: 6–8 years
February and October January to April
Qualifications
PhD (MPhil also available)
Duration
Full-time: 3–4 years
Part-time: 6–8 years
Start dates
February and October
Application period
January to April

Stellar astrophysics is a major facet of Astronomy research at the OU. We use a variety of methods, including theoretical investigations employing sophisticated population synthesis codes and observations made across the electromagnetic spectrum with world-leading facilities including The European Southern Observatory&/postgraduate/research-degrees/topic/stellar-astrophysics/39;s Very Large Telescopes (VLT), the Hubble Space Telescope (HST) and the Atacama Large Millimetre Array (ALMA). We use our proprietary time share on the 10-meter Southern African Large Telescope (SALT) and also deploy our own fully autonomous robotic telescopes in Tenerife, PIRATE and COAST.

We have strengths in both multi-wavelength observational programmes as well as in theoretical and computer modelling studies. A critical mass of postgraduate students currently pursues projects in this area, supported by five academic supervisors.

Entry requirements

Minimum 2:1 undergraduate degree (or equivalent). If you are not a UK citizen, you may need to prove your .

Potential research projects

We welcome enquiries from prospective students in the following areas:

  • Studies of massive stars, including massive binaries
  • Searches for the electromagnetic counterparts of gravitational wave sources
  • Mining archival time-domain datasets: pulsating and eclipsing systems
  • Multi-wavelength observations of interacting compact binary stars
  • Evolution of compact binaries
  • Synthetic stellar and binary populations
  • Exoplanet host stars

Please also see further opportunities.

Current/recent research projects

  • The life cycles of massive stars, including progenitors of gravitational wave sources
  • The identification and classification of variability in SuperWASP stars
  • 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
  • Stellar activity and star-planet interactions in planet host stars
  • Doppler tomography of star spots and implications for exoplanet searches

Potential supervisors

Fees and funding

UK fee International fee
Full-time: 拢4,786 per year Full-time: 拢15,698 per year
Part-time: 拢2,393 per year Part-time: 拢7,849 per year

Some of our research students are funded via the UKRI Science and Technology Facilities Council (STFC) Doctoral Training Partnership; others are self-funded.

For detailed information about fees and funding, visit Fees and studentships.

To see current funded studentship vacancies across all research areas, see .

Links

Antenna of radio telescope
 

How to apply

Get in touch

If you have an enquiry specific to this research topic, please contact:

Administrative support

Email: STEM SPS PHD
Phone: +44 (0)1908 653796

Apply now

Please review the application process if you’re interested in applying for this research topic.