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dc.contributor.authorBuser, R
dc.contributor.authorKaraali, S
dc.contributor.authorRong, JX
dc.date.accessioned2021-03-03T07:51:05Z
dc.date.available2021-03-03T07:51:05Z
dc.date.issued1999
dc.identifier.citationBuser R., Rong J., Karaali S., "The new Basel high-latitude field star survey of the Galaxy - II. The thick disk component: density structure, luminosity function, and metallicity distribution", ASTRONOMY & ASTROPHYSICS, cilt.348, sa.1, ss.98-112, 1999
dc.identifier.issn0004-6361
dc.identifier.othervv_1032021
dc.identifier.otherav_143e1c94-a080-4019-8290-1077a7e1f912
dc.identifier.urihttp://hdl.handle.net/20.500.12627/19008
dc.description.abstractWe present an expanded and refined analysis of the Galactic thick disk as observed in seven fields of the new Basel RGU star count and color survey data. Based on the optimized structural models which were obtained in the initial analysis (Buser et al. 1998a, hereafter Paper I), we now employ the same systematic least-squares algorithm, introducing more realistic luminosity functions for each population component, applying a more adequate matrix of color transformations in simulating the data, and extending the structural parameter ranges in order to determine improved characteristics of the thick-disk model.
dc.language.isoeng
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleThe new Basel high-latitude field star survey of the Galaxy - II. The thick disk component: density structure, luminosity function, and metallicity distribution
dc.typeMakale
dc.relation.journalASTRONOMY & ASTROPHYSICS
dc.contributor.department, ,
dc.identifier.volume348
dc.identifier.issue1
dc.identifier.startpage98
dc.identifier.endpage112
dc.contributor.firstauthorID123674


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