`Comparing the Predicted Abell/ACO Cluster & the MarkIII Galaxy Density and Velocity Fields', Contribution to the Wide Field Spectroscopy Meeting held in Athens, 20-24 May 1996

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dc.creatorPlionis, M.
dc.creatorBranchini, E.
dc.creatorZehavi, I.
dc.creatorDekel, A.
dc.date1996-09-20
dc.date.accessioned2026-07-07T02:21:57Z
dc.date.available2026-07-07T02:21:57Z
dc.descriptionWe compare the predicted Abell/ACO cluster density and velocity fields, using linear theory, with that based on the MarkIII catalog and the POTENT machinery within 7000 km/sec. Both density & velocity fields are in good qualitative agreement indicating that apart from a linear biasing factor the optical Abell/ACO clusters do trace the underlying mass distribution quite well.
dc.description4 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/9609142
dc.identifierhttp://arxiv.org/abs/astro-ph/9609142
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10694
dc.subjectAstrophysics
dc.title`Comparing the Predicted Abell/ACO Cluster & the MarkIII Galaxy Density and Velocity Fields', Contribution to the Wide Field Spectroscopy Meeting held in Athens, 20-24 May 1996
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