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Metallicity Gradients in Elliptical Galaxies

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dc.contributor.author Hanlan, Patricia C. en_US
dc.contributor.author Schombert, James M. en_US
dc.contributor.author Barsony, Mary en_US
dc.contributor.author Rakos, Karl D. en_US
dc.date.accessioned 2004-10-06T01:49:14Z
dc.date.available 2004-10-06T01:49:14Z
dc.date.issued 1993-01-25 en_US
dc.identifier.citation USA en_US
dc.identifier.clearanceno 93-0571 en_US
dc.identifier.uri http://hdl.handle.net/2014/35043
dc.description.abstract The study of metalicity gradients is an examination of the relics of the first epoch of star formation and, thus, another issue that metallicity gradients can address is the relationship between chemical and dynamical evolution during the initial phase of star formation. en_US
dc.format.extent 1309291 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other elliptical galaxies photometry evolution formation-mass-luminosity en_US
dc.title Metallicity Gradients in Elliptical Galaxies en_US


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