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Physical properties of simulated galaxy populations at z = 2 – I. Effect of metal-line cooling and feedback from star formation and AGN

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Dalla Vecchia,  Claudio
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Haas, M. R., Schaye, J., Booth, C. M., Dalla Vecchia, C., Springel, V., Theuns, T., et al. (2013). Physical properties of simulated galaxy populations at z = 2 – I. Effect of metal-line cooling and feedback from star formation and AGN. Monthly Notices of the Royal Astronomical Society, 435(4), 2931-2954. doi:10.1093/mnras/stt1487.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0015-8A5D-5
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