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Basic calibrations of the photographic RGU system IV. Metal-poor subgiant and giant stars

dc.contributor.authorRong, JX
dc.contributor.authorAk, SG
dc.contributor.authorWestera, P
dc.contributor.authorKaratas, Y
dc.contributor.authorLejeune, T
dc.contributor.authorBuser, R
dc.date.accessioned2021-03-06T20:45:26Z
dc.date.available2021-03-06T20:45:26Z
dc.date.issued2000
dc.identifier.citationBuser R., Karatas Y., Lejeune T., Rong J., Westera P., Ak S., "Basic calibrations of the photographic RGU system IV. Metal-poor subgiant and giant stars", ASTRONOMY & ASTROPHYSICS, cilt.357, ss.988-993, 2000
dc.identifier.issn0004-6361
dc.identifier.othervv_1032021
dc.identifier.otherav_fb90b2c0-84f3-4b8b-b68a-9e6e4ee1d663
dc.identifier.urihttp://hdl.handle.net/20.500.12627/164708
dc.description.abstractWe present a large grid of theoretical color-absolute magnitude and two-color diagrams in the RGU photometric system. The grid comprises wide ranges of stellar ages and physical parameters, and was computed using the YALE isochrones (Demarque et al. 1996) combined with the most recent version of the Basel Stellar Library (hereafter BaSeL) of color-calibrated theoretical model-atmosphere flux distributions (Lejeune et al. 2000).
dc.language.isoeng
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleBasic calibrations of the photographic RGU system IV. Metal-poor subgiant and giant stars
dc.typeMakale
dc.relation.journalASTRONOMY & ASTROPHYSICS
dc.contributor.department, ,
dc.identifier.volume357
dc.identifier.issue3
dc.identifier.startpage988
dc.identifier.endpage993
dc.contributor.firstauthorID125691


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