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dc.contributor.authorBuser, Roland
dc.contributor.authorKaraali, Salih
dc.contributor.authorBilir, Selçuk
dc.contributor.authorYaz, Esma
dc.contributor.authorHamzaoğlu, Esat
dc.date.accessioned2021-03-05T17:47:52Z
dc.date.available2021-03-05T17:47:52Z
dc.date.issued2007
dc.identifier.citationKaraali S., Bilir S., Yaz E., Hamzaoğlu E., Buser R., "Volume-limited dependent Galactic model parameters", PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA, cilt.24, ss.208-219, 2007
dc.identifier.issn1323-3580
dc.identifier.otherav_c7433ca8-d3ec-47dc-b922-777e2ea1adf6
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/132085
dc.identifier.urihttps://doi.org/10.1071/as07006
dc.description.abstractWe estimate 34 sets of Galactic model parameters for three intermediate-latitude fields with Galactic longitudes l = 60 degrees, l = 90 degrees, and l= 180 degrees, and we discussed their dependence on the volume. Also, we confirm the variation of these parameters with absolute magnitude and Galactic longitude. The star samples in two fields are restricted with bright and unit absolute-magnitude intervals, 4 < M-g <= 5, and 5 < M-g <= 6, whereas for the third field (l= 60 degrees) a larger absolute-magnitude interval is adopted, 4 < M-g <= 10. The limiting apparent magnitudes of the star samples are g(0) = 15 and g(0) = 22.5 mag, which provide space densities within distances in the line of sight of similar to 0.9 and 25 kpc.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectAstronomi ve Astrofizik
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectFizik
dc.subjectTemel Bilimler
dc.titleVolume-limited dependent Galactic model parameters
dc.typeMakale
dc.relation.journalPUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA
dc.contributor.departmentBeykent Üniversitesi , ,
dc.identifier.volume24
dc.identifier.issue4
dc.identifier.startpage208
dc.identifier.endpage219
dc.contributor.firstauthorID67442


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