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hal.structure.identifierAstronomical observatory of Odessa National University [Odessa]
dc.contributor.authorKOVTYUKH, V. V.
hal.structure.identifierAstronomical observatory of Odessa National University [Odessa]
dc.contributor.authorCHEKHONADSKIKH, F. A.
hal.structure.identifierDepartment of Astronomy, Case Western Reserve University,
dc.contributor.authorLUCK, R. E.
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierUniversité Sciences et Technologies - Bordeaux 1 [UB]
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
dc.contributor.authorSOUBIRAN, C.
dc.contributor.authorYASINSKAYA, M. P.
hal.structure.identifierOdessa Astronomical Observatory
dc.contributor.authorBELIK, S. I.
dc.date.issued2010
dc.identifier.issn0035-8711
dc.description.abstractEnLuminous FG supergiants can be used as extragalactic distance indicators. In order to fully exploit the properties of these bright stars, we must first learn how to measure their luminosities. Based primarily on classical Cepheids and supergiants in clusters and OB associations, we have derived 80 empirical relations connecting the line depth ratios of FeII/FeI lines with the absolute magnitudes Mv and the effective temperatures Teff. These relations have been applied to estimate the absolute magnitudes of 98 FG supergiants with an error of +/-0.26mag. The application range of our calibrations is spectral types F2-G8 and luminosity classes I and II (absolute magnitudes Mv, -0.5 to -8 mag). A comparison of our Mv determinations with values from the literature shows good agreement.
dc.language.isoen
dc.publisherOxford University Press (OUP): Policy P - Oxford Open Option A
dc.rights.urihttp://creativecommons.org/licenses/by/
dc.subject.enstars: fundamental parameters
dc.subject.ensupergiants
dc.subject.enstars: variables: Cepheids
dc.typeArticle de revue
dc.identifier.doi10.1111/J.1365-2966.2010.17217.X
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.subject.halPlanète et Univers [physics]
bordeaux.journalMonthly Notices of the Royal Astronomical Society
bordeaux.page1568–1575
bordeaux.volume408
bordeaux.peerReviewedoui
hal.identifierhal-00521973
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00521973v1
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