A Unique Mass Function from Galaxies to Clusters ?

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dc.contributor.areaPhysicsen_US
dc.contributor.authorGiuricin, Giuliano
dc.contributor.authorMardirossian, Fabio
dc.contributor.authorMezzetti, Marino
dc.contributor.authorPersic, Massimo
dc.contributor.authorSalucci, Paolo
dc.contributor.departmentAstrophysicsen_US
dc.date.accessioned2012-08-02T11:23:28Z
dc.date.available2012-08-02T11:23:28Z
dc.date.issued1993-08-11
dc.description9 pages (2 figures not included, available upon request), LATEX, SISSA Ref. 132/93/Aen_US
dc.description.abstractWe present an observational mass function ranging from galaxies to massive galaxy clusters, derived from direct dynamical mass estimates. Our mass function shows, in the low-mass range of galaxies and groups, a behaviour in agreement with that of standard CDM (n=-2), while in the high-mass range (clusters) our mass function is shallower (and thus contains more power) than standard CDM; it also results shallower than the recent mass function by Bahcall & Cen (1993, ApJ 407, L49).en_US
dc.identifier.urihttps://openscience.sissa.it/handle/1963/6087
dc.language.isoenen_US
dc.miur.area-1en_US
dc.publisherSISSAen_US
dc.relation.ispartofseriesarXiv:astro-ph/9308015v1;
dc.relation.ispartofseriesSISSA;132/1993/A
dc.titleA Unique Mass Function from Galaxies to Clusters ?en_US
dc.typePreprinten_US
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