Galaxy groups and binaries and the value of omega?

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dc.contributor.authorMorgan, Charles Gradyen_US
dc.date.accessioned2024-08-14T22:53:26Z
dc.date.available2024-08-14T22:53:26Z
dc.date.copyright1986en_US
dc.date.issued1986
dc.degree.departmentDepartment of Physics
dc.degree.departmentDepartment of Physics and Astronomy
dc.degree.levelMaster of Science M.Sc.en
dc.description.abstractA new technique which uses Oo as an input variable. for identifying gravitationally bound, dynamically isolated virialized groups of galaxies £ram a magnitude limited catalog is developed. The technique has been applied to the CfA redshift survey. In this thesis only the binary systems have been analyzed. Using a self-consistency argument. a value of Oo = 0.03 ~ 0.01 was obtained.
dc.format.extent182 pages
dc.identifier.urihttps://hdl.handle.net/1828/19037
dc.rightsAvailable to the World Wide Weben_US
dc.titleGalaxy groups and binaries and the value of omega?en_US
dc.typeThesisen_US

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