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Metal-poor turnoff and subgiant field stars in the Galaxy - I. RGU photometry in a high-latitude field near M101

dc.contributor.authorBuser, Roland
dc.contributor.authorKaraali, Salih
dc.contributor.authorAk, Serap
dc.date.accessioned2021-03-04T11:05:47Z
dc.date.available2021-03-04T11:05:47Z
dc.date.issued1998
dc.identifier.citationAk S., Karaali S., Buser R., "Metal-poor turnoff and subgiant field stars in the Galaxy - I. RGU photometry in a high-latitude field near M101", ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, cilt.131, sa.2, ss.345-354, 1998
dc.identifier.issn0365-0138
dc.identifier.otherav_709a8e18-699e-4e8e-b162-3a9675dbf0fe
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/77597
dc.identifier.urihttps://doi.org/10.1051/aas:1998429
dc.description.abstractPhotographic RGU photometry for about 1800 stars down to a limiting G-magnitude of 19.5 in a high-latitude field ((l, b) = (101 degrees, +60 degrees)) near the galaxy M101 is investigated. We use an improved variant of the classical three-color method which is based on recent UBV-RGU-photometric transforms and calibrations (Buser 1988; Buser & Fenkart 1990) and on models of the stellar density distributions of the Galactic population components.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectAstronomi ve Astrofizik
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectFizik
dc.subjectTemel Bilimler
dc.titleMetal-poor turnoff and subgiant field stars in the Galaxy - I. RGU photometry in a high-latitude field near M101
dc.typeMakale
dc.relation.journalASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES
dc.contributor.department, ,
dc.identifier.volume131
dc.identifier.issue2
dc.identifier.startpage345
dc.identifier.endpage354
dc.contributor.firstauthorID55222


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