Emergence of Filamentary Structure in Cosmological Gravitational Clustering
暂无分享,去创建一个
[1] P. Coles,et al. Approximation methods for non-linear gravitational clustering , 1995, astro-ph/9505005.
[2] Pauls,et al. The shape of the first collapsed objects. , 1994, Physical review letters.
[3] P. Coles,et al. Quantifying the geometry of large-scale structure , 1995 .
[4] A. Klypin,et al. Percolation technique for galaxy clustering , 1993 .
[5] A. Melott,et al. Controlled experiments in cosmological gravitational clustering , 1993 .
[6] A. Babul,et al. A quantitative measure of structure in the three-dimensional galaxy distribution : sheets and filaments , 1992 .
[7] S. Shandarin,et al. Percolation analysis of nonlinear structures in scale-free two-dimensional simulations , 1992 .
[8] John P. Huchra,et al. Measures of large-scale structure in the CfA redshift survey slices , 1991 .
[9] A. Klypin,et al. Three-dimensional numerical model of the formation of large-scale structure in the Universe , 1983 .
[10] Y. Zel’dovich,et al. The large scale structure of the universe I. General properties. One-and two-dimensional models , 1982 .