Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-30T10:47:14.813Z Has data issue: false hasContentIssue false

Large-Scale Structure Among Abell Clusters and Comparisons to Models

Published online by Cambridge University Press:  03 August 2017

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Copyright
Copyright © Reidel 1988