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An examination of recent transformations to the BV(RI)C photometric system from the perspective of stellar models for old stars

VandenBerg, Don A.; Casagrande, Luca; Stetson, Peter B

Description

Isochrones for ages ≳4 Gyr and metallicities in the range -2.5 ≲ [Fe/H] ≲ +0.3 that take the diffusion of helium and recent advances in stellar physics into account are compared with observations in the Johnson-Cousins BV(RI)C photometric system for

dc.contributor.authorVandenBerg, Don A.
dc.contributor.authorCasagrande, Luca
dc.contributor.authorStetson, Peter B
dc.date.accessioned2015-12-13T22:44:56Z
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/79534
dc.description.abstractIsochrones for ages ≳4 Gyr and metallicities in the range -2.5 ≲ [Fe/H] ≲ +0.3 that take the diffusion of helium and recent advances in stellar physics into account are compared with observations in the Johnson-Cousins BV(RI)C photometric system for
dc.publisherUniversity of Chicago Press
dc.sourceAstronomical Journal
dc.titleAn examination of recent transformations to the BV(RI)C photometric system from the perspective of stellar models for old stars
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume140
dc.date.issued2010
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB7956
local.type.statusPublished Version
local.contributor.affiliationVandenBerg, Don A., University of Victoria
local.contributor.affiliationCasagrande, Luca, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationStetson, Peter B, National Research Council of Canada
local.description.embargo2037-12-31
local.bibliographicCitation.issue4
local.bibliographicCitation.startpage1020
local.bibliographicCitation.lastpage1037
local.identifier.doi10.1088/0004-6256/140/4/1020
dc.date.updated2015-12-11T10:18:30Z
local.identifier.scopusID2-s2.0-78049337808
local.identifier.thomsonID000281722500012
CollectionsANU Research Publications

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