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Separation of dwarf and giant stars with ROTSE-IIId

dc.contributor.authorBilir, S.
dc.contributor.authorGuver, T.
dc.contributor.authorAslan, M.
dc.date.accessioned2021-03-05T18:45:59Z
dc.date.available2021-03-05T18:45:59Z
dc.date.issued2006
dc.identifier.citationBilir S., Guver T., Aslan M., "Separation of dwarf and giant stars with ROTSE-IIId", ASTRONOMISCHE NACHRICHTEN, cilt.327, ss.693-697, 2006
dc.identifier.issn0004-6337
dc.identifier.othervv_1032021
dc.identifier.otherav_cbe94e15-2edc-4581-a728-f461174bf123
dc.identifier.urihttp://hdl.handle.net/20.500.12627/135033
dc.identifier.urihttps://doi.org/10.1002/asna.200510614
dc.description.abstract136 stars which were known to be members of the open cluster NGC 752 were observed at the R band with the ROTSE-IIId telescope located at the Turkish National Observatory (TUG) site. The data had been evaluated together with BV and 2MASS photometric data. A new practical method for separating dwarf and giant was described and applied. Evaluating the colour magnitude-diagrams with Padova isochrones revealed for the open cluster NGC 752 a metallicity similar to the Sun and an age of 1.41 +/- 0.20 Gyr. g 2006 WILEY-VCH Verlag GmbH& Co. KGaA, Weinheim.
dc.language.isoeng
dc.subjectFizik
dc.subjectTemel Bilimler
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectAstronomi ve Astrofizik
dc.titleSeparation of dwarf and giant stars with ROTSE-IIId
dc.typeMakale
dc.relation.journalASTRONOMISCHE NACHRICHTEN
dc.contributor.departmentİstanbul Üniversitesi , Cerrahpaşa Tıp Fakültesi , Mikrobiyoloji
dc.identifier.volume327
dc.identifier.issue7
dc.identifier.startpage693
dc.identifier.endpage697
dc.contributor.firstauthorID177034


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