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Narrow-band photometry and the stellar populations in elliptical galaxies
dc.contributor.authorRakos, Karl D.en_US
dc.contributor.authorKreidl, Tobias J.en_US
dc.contributor.authorSchombert, James M.en_US
dc.date.accessioned2006-09-08T19:43:50Z
dc.date.available2006-09-08T19:43:50Z
dc.date.issued1990-08en_US
dc.identifier.citationRakos, Karl D.; Kreidl, Tobias J.; Schombert, James M.; (1990). "Narrow-band photometry and the stellar populations in elliptical galaxies." Astrophysics and Space Science 170 (1-2): 239-244. <http://hdl.handle.net/2027.42/41874>en_US
dc.identifier.issn0004-640Xen_US
dc.identifier.issn1572-946Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/41874
dc.description.abstractThe modified Strömgren uvby filter system, which has been used to investigate the spectrophotometric evolution of elliptical galaxies, is also found to be a powerful tool for the determination of stellar parameters in elliptical galaxies, especially metal content and the stellar type of the dominant population. We present an introduction to the behaviour of the filter system based on comparison to stellar libraries and then explore the results with respect to composite systems: globular clusters, spirals, and ellipticals.en_US
dc.format.extent311595 bytes
dc.format.extent3115 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherKluwer Academic Publishers; Springer Science+Business Mediaen_US
dc.subject.otherPhysicsen_US
dc.subject.otherAstronomyen_US
dc.titleNarrow-band photometry and the stellar populations in elliptical galaxiesen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDept. of Astronomy, University of Michigan, Ann Arbor, Michigan, U.S.A.en_US
dc.contributor.affiliationotherInstitute for Astronomy, University of Vienna, Austriaen_US
dc.contributor.affiliationotherLowell Observatory, Flagstaff, Arizona, U.S.A.en_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/41874/1/10509_2004_Article_BF00652674.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF00652674en_US
dc.identifier.sourceAstrophysics and Space Scienceen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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