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Virgo supercluster and the mean mass density of the Universe

Journal Article · · Astrophys. J., Lett. Ed.; (United States)
DOI:https://doi.org/10.1086/183269· OSTI ID:5071457
Recent measurements of the anisotropy of the microwave background radiation of the local Hubble flow suggest that the local group of galaxies has a motion of 300--500 km s/sup -1/ directed toward Virgo. If this velocity is generated by the Virgo supercluster, it provides a powerful test of the cosmological parameter ..cap omega... Using a catalog of redshift data complete to m/sub b/=14.0, we have computed the mean overdensity delta-bar toward the Virgo cluster to be approx.2.0 +- 0.3. When this result is combined with a nonlinear spherically symmetric flow model around Virgo, we derive ..cap omega.. approx. = 0.4 +- 0.1. Thus the measured mass-to-light ratio of the universe continues to rise with increasing scale size of measurement.
Research Organization:
Harvard-Smithsonian Center for Astrophysics
OSTI ID:
5071457
Journal Information:
Astrophys. J., Lett. Ed.; (United States), Journal Name: Astrophys. J., Lett. Ed.; (United States) Vol. 238:3; ISSN AJLEA
Country of Publication:
United States
Language:
English

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