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dc.contributor.authorTifft, W. G.
dc.date.accessioned2018-04-06T17:44:37Z
dc.date.available2018-04-06T17:44:37Z
dc.date.issued1972
dc.identifier.urihttp://hdl.handle.net/10150/627233
dc.description.abstractQuasi stellar absorption line redshifts are shown to be consistent with the redshift- magnitude band pattern concept. The redshifts in multiple redshift objects tend to concentrate at band crossings corresponding to the magnitude of each object.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 #0048en_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.subjectQuasarsen_US
dc.subjectAbsorption spectraen_US
dc.titleRedshift Magnitude Bands and Quasi Stellar Absorption Line Multiple Redshiftsen_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.dateFOA2018-04-06T17:44:37Z


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