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(-0.25)(+0.35). If the clustering of galaxies i...
मुख्य लेखकों: | Juszkiewicz, R, Ferreira, P, Feldman, H, Jaffe, A, Davis, M |
---|---|
स्वरूप: | Journal article |
भाषा: | English |
प्रकाशित: |
2000
|
समान संसाधन
-
Evidence for a low-density Universe from the relative velocities of
galaxies
द्वारा: Juszkiewicz, R, और अन्य
प्रकाशित: (2000) -
Measuring Ω with Galaxy Streaming Velocities
द्वारा: Ferreira, P, और अन्य
प्रकाशित: (1999) -
Streaming velocities as a dynamical estimator of Omega
द्वारा: Ferreira, P, और अन्य
प्रकाशित: (1998) -
Streaming velocities as a dynamical estimator of Omega
द्वारा: Ferreira, P, और अन्य
प्रकाशित: (1999) -
Power Spectrum Estimation from Peculiar Velocity Catalogues
द्वारा: Macaulay, E, और अन्य
प्रकाशित: (2011)