Globular Clusters and Galactic Chemical Evolution
Observational and theoretical studies of star clusters and their influence on the evolution of galaxies. (Supported by Marsden Fund research grant Element enrichment through mergers and stellar nucleosynthesis, Cottrell & Albrow.)
Pulsating Stars
Pulsating low mass supergiant stars are the precursors of proto-planetary nebulae. UC astrophysicists use facilities at the Mt John Observatory to study the pulsations and the shock waves produced in these stars.
Optical Design
UC astrophysicists have designed sophisticated optics and instrumentation for a number of medium - large telescopes both in New Zealand and overseas.
General Relativity and Theoretical Cosmology
UC astrophysicists work on theories of fundamental structure, black holes and dark energy.
Astroseismology
In much the same way that seismologists use earthquakes to deduce the structure of our planet, UC astrophysicists study the internal structure of stars by measuring tiny motions on their surfaces. (Supported by Marsden Fund research grant The music of the stars: Internal structure revealed through the surface vibrations of stars, Pollard & Cottrell.)
