The cosmic chemical evolution of galaxies
Lead Research Organisation:
University of Cambridge
Department Name: Physics
Abstract
The PhD thesis will consist in investigating the chemical evolution of galaxies across the cosmic epochs and, from this, constrain the role of different mechanisms and physical processes (e.g. galactic outflows, gas accretion, star formation efficiency) in galaxy formation and evolution. The thesis work will involve the analysis of data from current and forthcoming facilities (e.g. SDSS, JWST and MOONS) and also the development of models for the data interpretation, including the comparison with the prediction of cosmological numerical simulations.
Organisations
Publications
Baker W
(2023)
The molecular gas main sequence and Schmidt-Kennicutt relation are fundamental, the star-forming main sequence is a (useful) byproduct
in Monthly Notices of the Royal Astronomical Society
Baker W
(2023)
Stellar mass, not dynamical mass nor gravitational potential, drives the mass-metallicity relationship
in Monthly Notices of the Royal Astronomical Society
Baker W
(2023)
The metallicity's fundamental dependence on both local and global galactic quantities
in Monthly Notices of the Royal Astronomical Society
Baker W
(2022)
The ALMaQUEST survey IX: the nature of the resolved star forming main sequence
in Monthly Notices of the Royal Astronomical Society
Studentship Projects
Project Reference | Relationship | Related To | Start | End | Student Name |
---|---|---|---|---|---|
ST/R504671/1 | 30/09/2017 | 29/09/2021 | |||
2440936 | Studentship | ST/R504671/1 | 30/09/2020 | 31/03/2024 | William Baker |
ST/V506606/1 | 30/09/2020 | 29/09/2024 | |||
2440936 | Studentship | ST/V506606/1 | 30/09/2020 | 31/03/2024 | William Baker |