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Luminosity-colour relations for red clump stars

dc.contributor.authorBilir, Selçuk
dc.contributor.authorCakmak, H.
dc.contributor.authorOnal, Özgecan
dc.contributor.authorCabrera-Lavers, Antonio
dc.contributor.authorKaraali, S.
dc.date.accessioned2021-03-03T18:55:33Z
dc.date.available2021-03-03T18:55:33Z
dc.date.issued2013
dc.identifier.citationBilir S., Onal Ö., Karaali S., Cabrera-Lavers A., Cakmak H., "Luminosity-colour relations for red clump stars", ASTROPHYSICS AND SPACE SCIENCE, cilt.344, sa.2, ss.417-427, 2013
dc.identifier.issn0004-640X
dc.identifier.otherav_51c23ceb-1adc-431f-8dcf-5c93cf95a67e
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/58103
dc.identifier.urihttps://doi.org/10.1007/s10509-012-1342-9
dc.description.abstractWe calibrated the absolute magnitudes M (V) , M (J) , and M (g) of red clump stars in terms of colours. M (V) and M (g) are strongly dependent on colour, while the dependence of M (J) and on colour is rather weak. The calibration of the absolute magnitudes M (V) and is tested on 101 RC stars in the field SA 141. The Galactic model parameters estimated with this sample are in good agreement with earlier studies.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectAstronomi ve Astrofizik
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectFizik
dc.subjectTemel Bilimler
dc.titleLuminosity-colour relations for red clump stars
dc.typeMakale
dc.relation.journalASTROPHYSICS AND SPACE SCIENCE
dc.contributor.department, ,
dc.identifier.volume344
dc.identifier.issue2
dc.identifier.startpage417
dc.identifier.endpage427
dc.contributor.firstauthorID67510


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