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Absolute magnitudes for late-type dwarf stars for Sloan photometry

dc.contributor.authorTunçel, Sabiha
dc.contributor.authorKaraali, Salih
dc.contributor.authorBilir, Selçuk
dc.date.accessioned2021-03-04T11:19:23Z
dc.date.available2021-03-04T11:19:23Z
dc.date.issued2005
dc.identifier.citationBilir S., Karaali S., Tunçel S., "Absolute magnitudes for late-type dwarf stars for Sloan photometry", ASTRONOMISCHE NACHRICHTEN, cilt.326, sa.5, ss.321-331, 2005
dc.identifier.issn0004-6337
dc.identifier.otherav_71c7d93a-d100-4bf0-a72b-c2fc7d0bccd5
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/78332
dc.identifier.urihttps://doi.org/10.1002/asna.200510358
dc.description.abstractWe present a new formula for absolute magnitude determination for late-type dwarf stars as a function of (g - r) and (r - i) for Sloan photometry. The absolute magnitudes estimated by this approach are brighter than those estimated by colour-magnitude diagrams, and they reduce the luminosity function rather close to the luminosity function of Hipparcos.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectAstronomi ve Astrofizik
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectFizik
dc.subjectTemel Bilimler
dc.titleAbsolute magnitudes for late-type dwarf stars for Sloan photometry
dc.typeMakale
dc.relation.journalASTRONOMISCHE NACHRICHTEN
dc.contributor.departmentİstanbul Üniversitesi , ,
dc.identifier.volume326
dc.identifier.issue5
dc.identifier.startpage321
dc.identifier.endpage331
dc.contributor.firstauthorID67435


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