Kim, J.-h., O. Agertz, R. Teyssier, M. J. Butler, D. Ceverino, J.-H. Choi, R. Feldmann, B. W. Keller, A. Lupi, T. Quinn, Y. Revaz, S. Wallace, N. Y. Gnedin, S. N. Leitner, S. Shen, B. D. Smith, R. Thompson, M. J. Turk, T. Abel, K. S. Arraki, S. M. Benincasa, S. Chakrabarti, C. DeGraf, A. Dekel, N. J. Goldbaum, P. F. Hopkins, C. B. Hummels, A. Klypin, H. Li, P. Madau, N. Mandelker, L. Mayer, K. Nagamine, S. Nickerson, B. W. O'Shea, J. R. Primack, S. Roca-Fàbrega, V. Semenov, I. Shimizu, C. M. Simpson, K. Todoroki, J. W. Wadsley, J. H. Wise and A. Collaboration: The AGORA High-resolution Galaxy Simulations Comparison Project. II. Isolated Disk Test. In: The Astrophysical Journal 833, 2, (2016).
url: http://adsabs.harvard.edu/abs/2016ApJ...833..202K
Agertz, O., B. Moore, J. Stadel, D. Potter, F. Miniati, J. Read, L. Mayer, A. Gawryszczak, A. Kravtosov, A. Nordlund, F. Pearce, V. Quilis, D. Rudd, V. Springel, J. Stone, E. Tasker, R. Teyssier, J. Wadsley and R. Walder: Fundamental differences between SPH and grid methods. In: Monthly Notices of the Royal Astronomical Society 380, 3, 963-978 (2007).
doi: 10.1111/j.1365-2966.2007.12183.x
http://edoc.mpg.de
The Max Planck Society does not take any responsibility for the content of this export.