Dr Gareth Few

Dr Gareth Few

Research Fellow

Faculty and Department

  • Faculty of Science and Engineering
  • Department of Physics and Mathematics

Summary

Gareth Few is a computational astrophysicist whose research interests are the formation and evolution of spiral galaxies.

Specifically, he focuses on the processes which shape galaxies, how different chemical elements are distributed within them, and the various processes that determine where stars form.

Gareth's simulations use some of the world's most powerful supercomputers, without which these sophisticated hydrodynamics models would be impossible.

He is active in science outreach, presenting science talks to schools, science clubs and the public as well as chairing the Beverley Café Scientifique and Hull branch of the British Science Association.

Recent outputs

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Journal Article

The horizon run 5 cosmological hydrodynamical simulation: probing galaxy formation from kilo- to gigaparsec scales

Lee, J., Shin, J., Snaith, O. N., Kim, Y., Few, C. G., Devriendt, J., …Park, C. (2021). The horizon run 5 cosmological hydrodynamical simulation: probing galaxy formation from kilo- to gigaparsec scales. The Astrophysical journal, 908(1), https://doi.org/10.3847/1538-4357/abd08b

The time evolution of the Milky Way's oxygen abundance gradient

Mollá, M., Díaz, Á. I., Cavichia, O., Gibson, B. K., Maciel, W. J., Costa, R. D., …Few, C. G. (2019). The time evolution of the Milky Way's oxygen abundance gradient. Monthly notices of the Royal Astronomical Society, 482(3), 3071-3088. https://doi.org/10.1093/mnras/sty2877

The role of stellar radial motions in shaping galaxy surface brightness profiles

Ruiz-Lara, T., Few, C. G., Florido, E., Gibson, B. K., Pérez, I., & Sánchez-Blázquez, P. (2017). The role of stellar radial motions in shaping galaxy surface brightness profiles. Astronomy and Astrophysics, 608, A126. https://doi.org/10.1051/0004-6361/201731485

The Gaia-ESO Survey: matching chemodynamical simulations to observations of the Milky Way

Thompson, B. B., Few, C. G., Bergemann, M., Gibson, B. K., MacFarlane, B. A., Serenelli, A., …Zaggia, S. (2018). The Gaia-ESO Survey: matching chemodynamical simulations to observations of the Milky Way. Monthly notices of the Royal Astronomical Society, 473(1), 185-197. https://doi.org/10.1093/MNRAS/STX2316

Working Paper

The Horizon Run 5 Cosmological Hydrodynamic Simulation: Probing Galaxy Formation from Kilo- to Giga-parsec Scales

Lee, J., Shin, J., Snaith, O. N., Kim, Y., Few, C. G., Devriendt, J., …Park, C. The Horizon Run 5 Cosmological Hydrodynamic Simulation: Probing Galaxy Formation from Kilo- to Giga-parsec Scales

Postgraduate supervision

Gareth welcomes applications from potential PhD or Masters candidates interested in galaxy simulations and galactic chemical evolution.