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Simulations of the galaxy population constrained by observations from z = 3 to the present day: implications for galactic winds and the fate of their ejecta

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Henriques,  Bruno M. B.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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White,  Simon D. M.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Lemson,  Gerard
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Henriques, B. M. B., White, S. D. M., Thomas, P. A., Angulo, R. E., Guo, Q., Lemson, G., et al. (2013). Simulations of the galaxy population constrained by observations from z = 3 to the present day: implications for galactic winds and the fate of their ejecta. Monthly Notices of the Royal Astronomical Society, 431(4), 3373-3395. doi:10.1093/mnras/stt415.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-741F-F
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