Splotch: visualizing cosmological simulations
暂无分享,去创建一个
S. Imboden | M. Reinecke | K. Dolag | C. Gheller | M. Reinecke | K.Dolag | C.Gheller | S. Imboden | Claudio Gheller | Silvano Imboden
[1] S. Borgani,et al. Simulation Techniques for Cosmological Simulations , 2008, 0801.1023.
[2] M. Meneghetti,et al. Simulating the physical properties of dark matter and gas inside the cosmic web , 2005, astro-ph/0511357.
[3] F. Shu. Physics of Astrophysics: Volume I Radiation , 1991 .
[4] V. Springel,et al. X‐ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulation , 2004 .
[5] J. Monaghan,et al. A refined particle method for astrophysical problems , 1985 .
[6] Padova,et al. Populating a cluster of galaxies - I. Results at z=0 , 2000, astro-ph/0012055.
[7] J. Monaghan,et al. Smoothed particle hydrodynamics: Theory and application to non-spherical stars , 1977 .
[8] V. Springel. The Cosmological simulation code GADGET-2 , 2005, astro-ph/0505010.
[9] L. Moscardini,et al. Hot and cooled baryons in smoothed particle hydrodynamic simulations of galaxy clusters: physics and numerics , 2005, astro-ph/0512506.
[10] Stefano Borgani,et al. X-ray clusters of galaxies as tracers of structure in the Universe , 2001, Nature.