论文信息 - Streaming Velocities and the Formation of Large‐scale Structure a - 字舞流文

Streaming Velocities and the Formation of Large‐scale Structure a

[1] David Burstein,et al. Potential, velocity, and density fields from redshift-distance samples: Application - Cosmography within 6000 kilometers per second , 1990 .

[2] Sandra M. Faber,et al. Potential, velocity and density fields from sparse and noisy redshift distance samples: Method , 1990 .

[3] K. Gorski,et al. Effect of the Great Attractor on the cosmic microwave background radiation , 1990, Nature.

[4] George Efstathiou,et al. Galaxy correlations on large scales , 1990 .

[5] E. Bertschinger. Cosmic Strings and Galaxy Formation a , 1989 .

[6] Edmund Bertschinger,et al. Recovering the full velocity and density fields from large-scale redshift-distance samples , 1989 .

[7] David Burstein,et al. Spectroscopy and photometry of elliptical galaxies. V - Galaxy streaming toward the new supergalactic center , 1988 .

[8] P. Peebles. Origin of the large-scale galaxy peculiar velocity field: a minimal isocurvature model , 1987, Nature.

[9] M. Rees,et al. Physical mechanisms for biased galaxy formation , 1987, Nature.

[10] J. Silk,et al. Dwarf galaxies, cold dark matter, and biased galaxy formation , 1986 .

[11] R. Sachs,et al. Perturbations of a Cosmological Model and Angular Variations of the Microwave Background , 1967 .