ArTS Archivio della ricerca di Trieste
ArTS è il sistema di gestione integrata dei dati della ricerca adottato dall' Università degli Studi di Trieste
EnglishThe 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.
| Titolo: | The mass function of clusters of galaxies |
| Autori: | |
| Data di pubblicazione: | 1993 |
| 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. |
| Handle: | http://hdl.handle.net/11368/2634726 |
| ISBN: | 2863321420 |
| URL: | http://adsabs.harvard.edu/abs/1993cvf..conf..515B |
| Appare nelle tipologie: | 4.1 Contributo in Atti Convegno (Proceeding) |
File in questo prodotto:
Non ci sono file associati a questo prodotto.
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.