Davies et al. (2020b)

Quenching and morphological evolution due to circumgalactic gas expulsion in a simulated galaxy with a controlled assembly history

Jonathan J. Davies, Robert A. Crain and Andrew Pontzen

Rotating views of an "organic" star-forming disc galaxy simulated with the EAGLE model, and two further realisations of the same system that have "genetically modified" initial conditions that yield earlier (GM-Early) or later (GM-Late) assembly.

The movie shows the dark matter halo, followed by the stars and star-forming gas in the central galaxy, at redshifts 0, 1 and 2.

The systematic adjustments to the halo assembly history have a dramatic effect on the properties of the central galaxy. Shifting the assembly to earlier times yields a quenched, spheroidal galaxy at the present day, while shifting the assembly to later times yields a more vigorously star-forming disc.

This movie is available for download here.

Produced using py-sphviewer.

Figures

Full-resolution figures from the paper. Click to view full-size.

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j.j.davies@ucl.ac.uk

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Jonathan Davies
Department of Physics and Astronomy
University College London
Gower Street
London WC1E 6BT

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