Evidence for a low-density Universe from the relative velocities of galaxies
The motions of galaxies can be used to constrain the cosmological density parameter Omega and the clustering amplitude of matter on large scales. The mean relative velocity of galaxy pairs, estimated from the Mark III survey, indicates that Omega = 0.35 +0.35/-0.25. If the clustering of galaxies is...
| Asıl Yazarlar: | , , , , |
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| Materyal Türü: | Journal article |
| Baskı/Yayın Bilgisi: |
2000
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