Fritze-von Alvensleben, Uta

[["dc.bibliographiccitation.firstpage","L19"],["dc.bibliographiccitation.issue","3"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.lastpage","L23"],["dc.bibliographiccitation.volume","443"],["dc.contributor.author","Bicker, J."],["dc.contributor.author","Fritze-von Alvensleben, Uta"],["dc.date.accessioned","2018-11-07T10:53:42Z"],["dc.date.available","2018-11-07T10:53:42Z"],["dc.date.issued","2005"],["dc.description.abstract","We present new calibrations of the widely used H-alpha, [OII], and UV luminosity vs. star formation rate (SFR) relations. Using our evolutionary, synthesis code GALEV we compute the different calibrations for 5 metallicities, from 1/50 solar up to 2.5 solar. We find significant changes in the calibrations for lower metallicities compared to the standard calibrations using solar input physics."],["dc.identifier.doi","10.1051/0004-6361:200500194"],["dc.identifier.isi","000233320000002"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/49404"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Edp Sciences S A"],["dc.relation.issn","0004-6361"],["dc.title","Metallicity dependent calibrations of flux based SFR tracers"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]

[["dc.bibliographiccitation.firstpage","893"],["dc.bibliographiccitation.issue","2"],["dc.bibliographiccitation.journal","Astrophysics and Space Science"],["dc.bibliographiccitation.lastpage","896"],["dc.bibliographiccitation.volume","284"],["dc.contributor.author","Fritze-von Alvensleben, Uta"],["dc.contributor.author","Weilbacher, P."],["dc.contributor.author","Bicker, J."],["dc.date.accessioned","2018-11-07T10:42:03Z"],["dc.date.available","2018-11-07T10:42:03Z"],["dc.date.issued","2003"],["dc.description.abstract","To account for the range of stellar metallicities in local galaxies and for the increasing importance of low metallicities at higher redshift we present chemically consistent models for the spectral and chemical evolution of galaxies over cosmological timescales. We discuss advantages, limitations and future prospects of our approach."],["dc.identifier.doi","10.1023/A:1024014800146"],["dc.identifier.isi","000183320500119"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/46692"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","Najko"],["dc.publisher","Springer"],["dc.publisher.place","Dordrecht"],["dc.relation.conference","Conference on the Appropriate Modellings of Galaxy Evolution from their Cosmological Formation to their Presently Observable Structures"],["dc.relation.eventlocation","KIEL, GERMANY"],["dc.relation.issn","1572-946X"],["dc.relation.issn","0004-640X"],["dc.title","Chemically consistent evolutionary synthesis"],["dc.type","conference_paper"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dspace.entity.type","Publication"]]