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Scaling relations between super-massive black holes, galaxies and dark matter halos
Thesis
Larkin, A. Scaling relations between super-massive black holes, galaxies and dark matter halos. https://keele-repository.worktribe.com/output/408536

The observed correlations between the masses of supermassive black holes (SMBH), MBH, with a gravitational influence on parsec scales, and properties of the host galaxy, measured on kiloparsec scales, strongly suggest that the SMBH and galaxy co-evol... Read More about Scaling relations between super-massive black holes, galaxies and dark matter halos.

Three-dimensional hydrodynamic simulations of deep convection in massive stars
Thesis
Cristini, A. Three-dimensional hydrodynamic simulations of deep convection in massive stars. https://keele-repository.worktribe.com/output/409991

Convection plays a key role in the evolution of massive stars. Despite many decades of work on this topic, the treatment of convection (convective boundary mixing in particular) is still one of the major uncertainties in stellar evolution modelling.... Read More about Three-dimensional hydrodynamic simulations of deep convection in massive stars.

The impact of supernova remnants on interstellar dust within the Large Magellanic Cloud
Thesis
Lakicevic, M. The impact of supernova remnants on interstellar dust within the Large Magellanic Cloud. https://keele-repository.worktribe.com/output/407293

This thesis presents the first population study of supernova remnants (SNRs) in one whole galaxy – the Large Magellanic Cloud (LMC) on submm and FIR wavelengths. The first part is about the dust production in supernovae (SNe) and SNRs, based on sever... Read More about The impact of supernova remnants on interstellar dust within the Large Magellanic Cloud.

Identifying and characterising young, nearby, low-mass members of stellar moving groups
Thesis
Binks, A. S. Identifying and characterising young, nearby, low-mass members of stellar moving groups. https://keele-repository.worktribe.com/output/407043

Since the early 1990s, several groups of comoving, coeval stars younger than 100Myr and within 100 pc have been revealed. Studying and identifying members in these ‘Nearby Young Moving Groups’ (MGs) is vital because they provide: well characterised s... Read More about Identifying and characterising young, nearby, low-mass members of stellar moving groups.

Spitzer Space Telescope observations of hot Jupiters
Thesis
Mahtani, D. P. Spitzer Space Telescope observations of hot Jupiters. https://keele-repository.worktribe.com/output/407058

Currently the Spitzer Space Telescope is the most reliable telescope for conducting secondary eclipse observations of exoplanets. The depth and the time of mid-eclipse are two important parameters that come from a secondary eclipse analysis. The ecli... Read More about Spitzer Space Telescope observations of hot Jupiters.

Kinematics and age spreads of the young star-forming region NGC 2264
Thesis
Dobson, A. Kinematics and age spreads of the young star-forming region NGC 2264. https://keele-repository.worktribe.com/output/407163

While stars are relatively well understood, the timescales on which they form are still debated. The young cluster NGC 2264 is an ideal region in which to test hypotheses about the timescale of star and cluster formation. Co-eval stars at any given e... Read More about Kinematics and age spreads of the young star-forming region NGC 2264.