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Large-Scale Structure Among Abell Clusters and Comparisons to Models

Published online by Cambridge University Press:  03 August 2017

David J. Batuski ,
Jack O. Burns  and
Adrian Melott
David J. Batuski
Affiliation:
Space Telescope Science Institute, Homewood Campus, Baltimore, MD 21218 USA
Jack O. Burns
Affiliation:
Institute for Astrophysics, Univ. of New Mexico, Albuquerque, NM 87131 USA
Adrian Melott
Affiliation:
Department of Physics and Astronomy, Univ. of Kansas, Lawrence, KS 66045 USA

Extract

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In a continuing redshift observation program, we have recently determined or confirmed the redshifts of 32 R ≥ 0 Abell clusters. With these data added to the previously measured cluster redshifts, there is now a sample of Abell clusters to z = 0.085 that is 92% complete in redshift measurements. The sample consists of 225 clusters in the North and South Galactic Caps, with latitude |b| > 30° to minimize obscuration effects. The longitude range 270° < l < 360° was also excluded for this sample because of an apparent large spur of galactic absorption.

Type
Appendix 1: Poster Papers
Information
Symposium - International Astronomical Union , Volume 130: Large Scale Structures of the Universe , 1988 , pp. 543
Copyright
Copyright © Reidel 1988