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dc.contributor.authorTifft, W. G.
dc.date.accessioned2018-04-06T22:58:27Z
dc.date.available2018-04-06T22:58:27Z
dc.date.issued1973-06
dc.identifier.citationAPJ 188: 221-232 (1974)en_US
dc.identifier.urihttp://hdl.handle.net/10150/627250
dc.description.abstractRedshift- magnitude bands as they occur in the Coma cluster are formally defined and the original bands as observed in 1972 are shown to have a likelihood of random occurance of only 0.005 independent of their direction. The properties of the Coma bands are transformed to m_p magnitudes and used to show that an independent sample of outlying Coma galaxies shows strong band related characteristics. The proper- ties of the Coma bands are then used to predict band properties for the A2199 cluster. The resultant power spectrum test of a preliminary A2199 sample shows agreement which has a random likelihood of occurance of only 0.001. The A2199 cluster also shows a band related morphological separation as in Coma.en_US
dc.language.isoen_USen_US
dc.publisherSteward Observatory, The University of Arizona (Tucson, Arizona)en_US
dc.relation.ispartofseriesPreprints of the Steward Observatory #0061en_US
dc.relation.urlhttp://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1974ApJ...188..221T&db_key=AST&data_type=HTML&format=&high=3ed65e9cd019639en_US
dc.rightsCopyright © All Rights Reserved.en_US
dc.sourceSteward Observatory Parker Library SO QB 4 .S752 ARCHen_US
dc.subjectRedshiften_US
dc.subjectMagnitudesen_US
dc.subjectClusters of galaxiesen_US
dc.titleThe Definition, Visibility, and Significance of Redshift-Magnitude Bandsen_US
dc.typetexten_US
dc.contributor.departmentUniv Arizona, Steward Observen_US
dc.description.collectioninformationThis title from the Steward Observatory Preprints collection is made available by the Steward Observatory Parker Library and the University Libraries, The University of Arizona. If you have questions about titles in this collection, please contact Parker Library librarian Betty Fridena, bfridena@as.arizona.edu.en_US
refterms.dateFOA2018-04-06T22:58:27Z


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