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Galactic model parameters for field giants separated from field dwarfs by their 2MASS and V apparent magnitudes

dc.contributor.authorKarataş, Yüksel
dc.contributor.authorGüver, Tolga
dc.contributor.authorKaraali, Salih
dc.contributor.authorBilir, Selçuk
dc.contributor.authorAk, Serap
dc.date.accessioned2021-03-05T12:38:08Z
dc.date.available2021-03-05T12:38:08Z
dc.date.issued2006
dc.identifier.citationBilir S., Karaali S., Güver T., Karataş Y., Ak S., "Galactic model parameters for field giants separated from field dwarfs by their 2MASS and V apparent magnitudes", ASTRONOMISCHE NACHRICHTEN, cilt.327, ss.72-81, 2006
dc.identifier.issn0004-6337
dc.identifier.othervv_1032021
dc.identifier.otherav_ae1bc635-b5d1-4a78-9493-0b5a0040d7c1
dc.identifier.urihttp://hdl.handle.net/20.500.12627/116167
dc.identifier.urihttps://doi.org/10.1002/asna.200510480
dc.description.abstractWe present a method which separates field dwarfs and field giants by their 2MASS and V apparent magnitudes. This method is based on spectroscopically selected standards and is hence reliable. We applied it to stars in two fields, SA 54 and SA 82, and we estimated a full set of Galactic model parameters for giants including their total local space density. Our results are in agreement with the ones given in the recent literature.
dc.language.isoeng
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler (SCI)
dc.subjectFizik
dc.subjectTemel Bilimler
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.titleGalactic model parameters for field giants separated from field dwarfs by their 2MASS and V apparent magnitudes
dc.typeMakale
dc.relation.journalASTRONOMISCHE NACHRICHTEN
dc.contributor.departmentİstanbul Üniversitesi , Fen Fakültesi , Astronomi Ve Uzay Bilimleri
dc.identifier.volume327
dc.identifier.issue1
dc.identifier.startpage72
dc.identifier.endpage81
dc.contributor.firstauthorID55230


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