Hot and cooled baryons in smoothed particle hydrodynamic simulations of galaxy 
clusters: physics and numerics

Borgani, S.; Dolag, K.; Murante, G.; Cheng, L. M.; Springel, V.; Diaferio, A.; Moscardini, L.; Tormen, G.; Tornatore, L.; Tozzi, P.

doi:10.1111/j.1365-2966.2006.10075.x

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Hot and cooled baryons in smoothed particle hydrodynamic simulations of galaxy clusters: physics and numerics

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Dolag, K.
Cosmology, MPI for Astrophysics, Max Planck Society;

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Springel, V.
Cosmology, MPI for Astrophysics, Max Planck Society;

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Borgani, S., Dolag, K., Murante, G., Cheng, L. M., Springel, V., Diaferio, A., Moscardini, L., Tormen, G., Tornatore, L., & Tozzi, P. (2006). Hot and cooled baryons in smoothed particle hydrodynamic simulations of galaxy clusters: physics and numerics. Monthly Notices of the Royal Astronomical Society, 367(4), 1641-1654. doi:10.1111/j.1365-2966.2006.10075.x.

引用: https://hdl.handle.net/11858/00-001M-0000-0011-AF6A-B

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