University of Birmingham Featured PhD Programmes
University of Kent Featured PhD Programmes
National University of Ireland, Galway Featured PhD Programmes
University of Southampton Featured PhD Programmes
University of Manchester Featured PhD Programmes

Sweeping galaxies clean: how do black holes drive powerful molecular outflows? (astronomy)

This project is no longer listed in the FindAPhD
database and may not be available.

Click here to search the FindAPhD database
for PhD studentship opportunities
  • Full or part time
    Dr T Davis
    Dr P Clark
  • Application Deadline
    No more applications being accepted
  • Competition Funded PhD Project (European/UK Students Only)
    Competition Funded PhD Project (European/UK Students Only)

Project Description

In order to reproduce the tight correlations observed between galaxies and the supermassive black holes that lie in their hearts, galaxy formation and evolution models require accretion powered active galactic nuclei (AGN) to drive large outflows and quench galaxies. In order to shut down star formation on short timescales these outflows must strongly affect the cold gas: destroying it, or driving it out of the galaxy entirely. Recently a series of observational studies have shown that AGN can drive cold gas from galaxies, however these studies leave a large number of open questions. This project aims to address these questions, using (magneto-)hydrodynamic simulations with molecular chemistry to predict the properties of cold gas in outflows, and how these properties change with e.g. differing ejection
mechanisms and gas conditions. Initially the student will explore simple molecular chemistry in the outflow, focusing on H2 and CO. The chemical networks for these species are already implemented in our version of the Arepo astrophysical fluid code. She/he will then have the opportunity to look at more complex species using a ’tracer particle’ method. The student can then compare these simulations with existing and new observational data (from world leading facilities such as the Atacama Large Millimetre/submillimetre Array) to shed light on these complex processes that shape the evolution of galaxies. The student who takes on this project will pick up a wide range of research skills, including numerical modelling (fluids codes/radiative transfer/chemical modelling) and observational techniques.

Funding Notes

The Science Technology Facilities Council welcomes applications from both UK and EU applicants.
Full awards (tuition fees plus maintenance stipend) are open to UK Nationals and EU students who can satisfy UK residency requirements. For more information visit:
The research project listed above is in competition with other projects for 2017/18; studentships will be awarded to the highest ranked applicants from all applications received. We reserve the right to close applications early should sufficient applications be received.

Related Subjects

How good is research at Cardiff University in Physics?

FTE Category A staff submitted: 19.50

Research output data provided by the Research Excellence Framework (REF)

Click here to see the results for all UK universities

FindAPhD. Copyright 2005-2019
All rights reserved.