The distribution of virial masses for nearby galaxy clusters is presented. The analysis is based on a data-set of 75 clusters, each with >20 members with measured redshifts within 1.5h^-1 Mpc. Having accounted for problems of incompleteness of the data-set, a power is finally fitted to the mass distribution. Constraints on the spectrum of primordial fluctuations are obtained.
The mass function of clusters of galaxies / A., B., Girardi, M., Giuricin, G., Mardirossian, F., Mezzetti, M.. - STAMPA. - (1993), pp. 515-516. (Cosmic Velocity Fields, 9th IAP Astrophysics Meeting Paris, France July 12-17, 1993).
The mass function of clusters of galaxies
GIRARDI, MARISA;GIURICIN, GIULIANO;MARDIROSSIAN, FABIO;MEZZETTI, MARINO
1993-01-01
Abstract
The distribution of virial masses for nearby galaxy clusters is presented. The analysis is based on a data-set of 75 clusters, each with >20 members with measured redshifts within 1.5h^-1 Mpc. Having accounted for problems of incompleteness of the data-set, a power is finally fitted to the mass distribution. Constraints on the spectrum of primordial fluctuations are obtained.File in questo prodotto:
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