A 140 Mpc Oscillation of the Abell Cluster Correlation Function

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dc.creatorSaar, Veikko
dc.creatorTago, Erik
dc.creatorEinasto, Jaan
dc.creatorEinasto, Maret
dc.creatorAndernach, Heinz
dc.date1995-05-11
dc.date.accessioned2026-07-07T02:19:46Z
dc.date.available2026-07-07T02:19:46Z
dc.descriptionWe have developed a parameter-independent method to detect local maxima of the two-point correlation function. By applying it to two samples of rich Abell clusters of galaxies with redshift limits z<0.08 and z<0.12 we detect three maxima centered at 150 Mpc, 300 Mpc and 430 Mpc with confidence levels 80% and higher. This sequence of fluctuations has an average interval of 140 Mpc, that can be explained by a power spectrum with a distinct peak at k=0.048+-0.005/Mpc.
dc.description8 pages, uuencoded compressed postscript, includes 6 figures, submitted to ApJ, abbreviated for the proceedings of the XXXth Moriond meeting
dc.identifierhttps://arxiv.org/abs/astro-ph/9505053
dc.identifierhttp://arxiv.org/abs/astro-ph/9505053
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9999
dc.subjectAstrophysics
dc.titleA 140 Mpc Oscillation of the Abell Cluster Correlation Function
dc.typetext

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