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dc.contributor.authorHaberzettl, Lutz
dc.date.accessioned2010-10-12T18:25:48Z
dc.date.available2010-10-12T18:25:48Z
dc.date.issued2005
dc.identifier.urihttp://hdl.handle.net/11858/00-1735-0000-0001-3123-0
dc.description.abstractI presented the first study of the SFH of LSB galaxies by using integrated spectra. The analyzed sample was derived during a search for LSBs in the HDFS. The selection was done using a new method based on the locations of the galaxies in the colorcolor diagrams. As shown by Haberzettl (1999), the LSB galaxies in the colorcolor diagrams do not follow the redshift tracks built by the HSB galaxies. In the colorcolor diagrams, these tracks represent the five standard Hubble types. The different locations of the selected LSB galaxies are a first hint for their different stellar population mix ...
dc.format.extent155 S.
dc.format.mimetypeapplication/pdf
dc.language.isodeu
dc.publisherUniv. Bochum
dc.rights.urihttp://e-docs.geo-leo.de/rights
dc.subject.ddc523
dc.subject.gokTEG 000
dc.subject.gokTIE 400
dc.titleStar formation history of low surface brightness galaxies in the HDFS
dc.typemonograph
dc.subject.gokverbalKosmogonie {Astronomie}
dc.subject.gokverbalSpektren und Leuchtkraft von Sternsystemen {Astronomie}
dc.identifier.doi10.23689/fidgeo-155
dc.identifier.ppn91577527
dc.identifier.urnurn:nbn:de:hbz:294-15163
dc.type.versionpublishedVersion
dc.relation.collectionAstronomie, Astrophysik, Weltraumforschung
dc.description.typethesis


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