Galaxies at High Redshifts
Yahil, A. · Lanzetta, K. M. · Fernandez-Soto, A.
Original · EN
Several conclusions have been reached over the last few years concerning high-redshift galaxies: (1) The excess of faint blue galaxies is due to dwarf galaxies. (2) Star formation peaks at redshifts z 1-2. (3) It appears to occur piecemeal in any given galaxy and there is no evidence for starbursting throughout a large 10 kpc galaxy. (4) There is significant and sharp diminution in the number of L* spiral galaxies at redshifts 1<z<2 and elliptical galaxies at redshifts 2.5<z<4. (5) It is increasingly more difficult to hide large high-redshift galaxies in universes with larger volumes per unit redshift, i.e., open or lambda models, which have lower deceleration parameters.
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