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dc.contributor.authorKaraali, S.
dc.contributor.authorBilir, Selçuk
dc.contributor.authorHamzaoglu, E.
dc.date.accessioned2021-03-03T08:31:52Z
dc.date.available2021-03-03T08:31:52Z
dc.date.issued2009
dc.identifier.citationKaraali S., Hamzaoglu E., Bilir S., "A universal vertical stellar density distribution law for the Galaxy", ASTROPHYSICS AND SPACE SCIENCE, cilt.324, sa.1, ss.23-30, 2009
dc.identifier.issn0004-640X
dc.identifier.otherav_1809aef1-0745-45d4-96a6-e7d78ff24b9d
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/21476
dc.identifier.urihttps://doi.org/10.1007/s10509-009-0149-9
dc.description.abstractWe reduced the observational logarithmic space densities in the vertical direction up to 8 kpc from the galactic plane, for stars with absolute magnitudes (5,6], (6,7] and [5,10] in the fields #0952+5245 and SA114, to a single exponential density law. One of three parameters in the quadratic expression of the density law corresponds to the local space density for stars with absolute magnitudes in question. There is no need of any definition for scaleheights or population types. We confirm with the arguments of non-discrete thin and thick discs for our Galaxy and propose a single structure up to several kiloparsecs from the galactic plane. The logarithmic space densities evaluated by this law for the ELAIS field fit to the observational ones. Whereas, there are considerable offsets for the logarithmic space densities produced by two sets of classical galactic model parameters from the observational ones, for the same field.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectAstronomi ve Astrofizik
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectFizik
dc.subjectTemel Bilimler
dc.titleA universal vertical stellar density distribution law for the Galaxy
dc.typeMakale
dc.relation.journalASTROPHYSICS AND SPACE SCIENCE
dc.contributor.departmentBeykent Üniversitesi , ,
dc.identifier.volume324
dc.identifier.issue1
dc.identifier.startpage23
dc.identifier.endpage30
dc.contributor.firstauthorID67477


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