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Galactic longitude dependent galactic model parameters

dc.contributor.authorYaz, Esma
dc.contributor.authorHamzaoğlu, Esat
dc.contributor.authorKaraali, Salih
dc.contributor.authorBilir, Selçuk
dc.contributor.authorAk, Serap
dc.date.accessioned2021-03-05T18:35:48Z
dc.date.available2021-03-05T18:35:48Z
dc.date.issued2006
dc.identifier.citationBilir S., Karaali S., Ak S., Yaz E., Hamzaoğlu E., "Galactic longitude dependent galactic model parameters", NEW ASTRONOMY, cilt.12, ss.234-245, 2006
dc.identifier.issn1384-1076
dc.identifier.othervv_1032021
dc.identifier.otherav_cb0dc6d5-5258-4e01-a0e6-74c0375d6e9e
dc.identifier.urihttp://hdl.handle.net/20.500.12627/134523
dc.identifier.urihttps://doi.org/10.1016/j.newast.2006.10.001
dc.description.abstractWe present the Galactic model parameters for thin disc estimated by Sloan Digital Sky Survey (SDSS) data of 14 940 stars with apparent magnitudes 16 = 220 pc (196 = 1900 pc (1561 <= h <= 2280 pc) respectively. This result would be useful to explain different numerical values claimed for those parameters obtained by different authors for the fields in different directions of the Galaxy. (c) 2006 Elsevier B.V. All rights reserved.
dc.language.isoeng
dc.subjectFizik
dc.subjectTemel Bilimler
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleGalactic longitude dependent galactic model parameters
dc.typeMakale
dc.relation.journalNEW ASTRONOMY
dc.contributor.departmentBeykent Üniversitesi , ,
dc.identifier.volume12
dc.identifier.issue3
dc.identifier.startpage234
dc.identifier.endpage245
dc.contributor.firstauthorID55236


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