Skip to main content

Research Repository

Advanced Search

Professor Adrian Jenkins' Outputs (4)

The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies (2017)
Journal Article
Barnes, D. J., Kay, S. T., Bahé, Y. M., Dalla Vecchia, C., McCarthy, I. G., Schaye, J., …White, S. D. (2017). The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies. Monthly Notices of the Royal Astronomical Society, 471(1), 1088-1106. https://doi.org/10.1093/mnras/stx1647

We introduce the Cluster-EAGLE (C-EAGLE) simulation project, a set of cosmological hydrodynamical zoom simulations of the formation of 30 galaxy clusters in the mass range of 1014 < M200/M⊙ < 1015.4 that incorporates the Hydrangea sample of Bahé et a... Read More about The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies.

The Hydrangea simulations: galaxy formation in and around massive clusters (2017)
Journal Article
Bahé, Y., Barnes, D., Dalla Vecchia, C., Kay, S., White, S., McCarthy, I., …Trayford, J. (2017). The Hydrangea simulations: galaxy formation in and around massive clusters. Monthly Notices of the Royal Astronomical Society, 470(4), 4186-4208. https://doi.org/10.1093/mnras/stx1403

We introduce the Hydrangea simulations, a suite of 24 cosmological hydrodynamic zoom-in simulations of massive galaxy clusters (M200c = 1014–1015.4 M⊙) with baryon particle masses of ∼106 M⊙. Designed to study the impact of the cluster environment on... Read More about The Hydrangea simulations: galaxy formation in and around massive clusters.

Knowing the unknowns: uncertainties in simple estimators of galactic dynamical masses (2017)
Journal Article
Campbell, D. J., Frenk, C. S., Jenkins, A., Eke, V. R., Navarro, J. F., Sawala, T., …Theuns, T. (2017). Knowing the unknowns: uncertainties in simple estimators of galactic dynamical masses. Monthly Notices of the Royal Astronomical Society, 469(2), 2335-2360. https://doi.org/10.1093/mnras/stx975

The observed stellar kinematics of dispersion-supported galaxies are often used to measure dynamical masses. Recently, several analytical relationships between the stellar line-of-sight velocity dispersion, the projected (2D) or deprojected (3D) half... Read More about Knowing the unknowns: uncertainties in simple estimators of galactic dynamical masses.

The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time (2017)
Journal Article
Grand, R., Gómez, F., Marinacci, F., Pakmor, R., Springel, V., Campbell, D., …White, S. (2017). The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time. Monthly Notices of the Royal Astronomical Society, 467(1), 179-207. https://doi.org/10.1093/mnras/stx071

We introduce a suite of 30 cosmological magneto-hydrodynamical zoom simulations of the formation of galaxies in isolated Milky Way mass dark haloes. These were carried out with the moving mesh code arepo, together with a comprehensive model for galax... Read More about The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time.