Galaxy formation
Implications of the isotropy of the cosmic microwave background on large and small angular scales for galaxy formation are reviewed. In primeval adiabatic fluctuations, a universe dominated by cold, weakly interacting nonbaryonic matter, e.g., the massive photino is postulated. A possible signature of photino annihilation in our galactic halo involves production of cosmic ray antiprotons. If the density is near its closure value, it is necessary to invoke a biasing mechanism for suppressing galaxy formation throughout most of the universe in order to reconcile the dark matter density with the lower astronomical determinations of the mean cosmological density. A mechanism utilizing the onset of primordial massive star formation to strip gaseous protogalaxies is described. Only the densest, early collapsing systems form luminous galaxies. (ESA)
- Research Organization:
- California Univ., Berkeley (USA)
- OSTI ID:
- 5605617
- Report Number(s):
- N-85-22321
- Resource Relation:
- Other Information: In ESA, plasma astrophys., 327-340 p., (N--85-22270 12-90)
- Country of Publication:
- United States
- Language:
- English
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