Dr Gareth Few

Dr Gareth Few

Lecturer

Faculty and Department

  • Faculty of Science and Engineering
  • School of Natural Sciences

Summary

Gareth Few is a computational astrophysicist with a background researching the formation and evolution of spiral galaxies and galactic chemical evolution using simulations.

After postdoctoral positions at the University of Exeter and the University of Hull he has devoted himself to excellence in physics education, teaching at Durham University and then returning to Hull as a lecturer.

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

Recent outputs

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Journal Article

Formation and Morphology of the First Galaxies in the Cosmic Morning

Park, C., Lee, J., Kim, J., Jeong, D., Pichon, C., Gibson, B. K., …Few, C. G. (2022). Formation and Morphology of the First Galaxies in the Cosmic Morning. The Astrophysical journal, 937(1), https://doi.org/10.3847/1538-4357/ac85b5

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), Article 11. 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

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

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