Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models

We compare global predictions from the eagle hydrodynamical simulation, and two semi-analytic (SA) models of galaxy formation, l-galaxies and galform. All three models include the key physical processes for the formation and evolution of galaxies and their parameters are calibrated against a small n...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2016-10, Vol.461 (4), p.3457-3482
Hauptverfasser:	Guo, Quan, Gonzalez-Perez, Violeta, Guo, Qi, Schaller, Matthieu, Furlong, Michelle, Bower, Richard G., Cole, Shaun, Crain, Robert A., Frenk, Carlos S., Helly, John C., Lacey, Cedric G., Lagos, Claudia del P., Mitchell, Peter, Schaye, Joop, Theuns, Tom
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Astronomy Comparative analysis Computer simulation Dark matter Fluid mechanics Galaxies Mathematical models Simulation Star formation rate Stars & galaxies Stellar evolution Stellar mass
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