Mo, Houjun.
Mo, Houjun, 1963-
Houjun Mo
VIAF ID: 40025466 ( Personal )
Permalink: http://viaf.org/viaf/40025466
Preferred Forms
- 100 0 _ ‡a Houjun Mo
- 200 _ | ‡a Mo ‡b Houjun
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- 100 1 _ ‡a Mo, Houjun
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- 100 1 _ ‡a Mo, Houjun
- 100 1 _ ‡a Mo, Houjun ‡d 1963-
- 100 1 _ ‡a Mo, Houjun ‡d 1963-
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4xx's: Alternate Name Forms (8)
Works
Title | Sources |
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analytic model for the gravitational clustering of dark matter haloes | |
Analytical approximations to the low-order statistics of dark matter distribution | |
Can morphological segregations of galaxies exist on 10h-1Mpc scales? | |
Constraints on the cosmic structure formation models from early formation of giant galaxies | |
The correlation function of clusters of galaxies and the amplitude of mass fluctuations in the universe | |
Correlation functions of galaxies with different weightings according to luminosity and mass implications for biased galaxy formation | |
The evolution of correlation functions and power spectra in gravitational clustering | |
formation of galactic disks | |
Galaxy formation and evolution, 2010: | |
Gaseous galactic halos and QSO absorption line systems | |
Geometrical analysis of galaxy clustering dependence on luminosity | |
High order correlations of peaks and halos a step toward understanding galaxy biasing | |
Lyman [alpha-absorption] at low redshifts and hot gas in galactic haloes | |
Mapping the universe statistical measures of the galaxy distribution | |
Percolation analysis and void probability functions of galaxies of different morphological type | |
percolation analysis of cluster superclasting | |
Probing pencil-beams in pancake-models | |
Proceedings of the Workshop on From Stars to Galaxies to the Universe, 1999: | |
Spatial correlation function and pairwise velocity dispersion of galaxies CDM models versus the LasCampanas Survey | |
A statistical discriminator among galaxy samples of different large-scale topology and geometry | |
The structure and clustering of Lyman break galaxies | |
Typical scales in the distribution of galaxies and clusters of galaxies from unnormalized pair counts |