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Stellar ages and convective cores in field main-sequence stars: First asteroseismic application to two kepler targets

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dc.contributor.authorAguirre, V Silva
dc.contributor.authorBasu, S
dc.contributor.authorBrandao, I M
dc.contributor.authorChristensen-Dalsgaard, J
dc.contributor.authorDeheuvels, S
dc.contributor.authorDogan, G
dc.contributor.authorMetcalfe, T S
dc.contributor.authorSerenelli, A. M.
dc.contributor.authorBallot, J
dc.contributor.authorChaplin, W. J.
dc.contributor.authorCunha, M S
dc.contributor.authorWeiss, A
dc.contributor.authorAppourchaux, T
dc.contributor.authorCasagrande, Luca
dc.date.accessioned2015-12-13T22:24:34Z
dc.date.issued2013
dc.date.updated2016-02-24T09:10:48Z
dc.description.abstractUsing asteroseismic data and stellar evolution models we obtain the first detection of a convective core in a Kepler field main-sequence star, putting a stringent constraint on the total size of the mixed zone and showing that extra mixing beyond the form
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/72786
dc.publisherIOP Publishing
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: asteroseismology; stars: fundamental parameters; stars: interiors; stars: oscillations
dc.titleStellar ages and convective cores in field main-sequence stars: First asteroseismic application to two kepler targets
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2
local.contributor.affiliationAguirre, V Silva, Aarhus University
local.contributor.affiliationBasu, S, Yale University
local.contributor.affiliationBrandao, I M , Universidade do Porto
local.contributor.affiliationChristensen-Dalsgaard, J, Aarhus University
local.contributor.affiliationDeheuvels, S, Yale University
local.contributor.affiliationDogan, G, High Altitude Observatory
local.contributor.affiliationMetcalfe, T S, University of Texas
local.contributor.affiliationSerenelli, A. M., Kavli Institute for Theoretical Physics
local.contributor.affiliationBallot, J, CNRS, Institut de Recherche en Astrophysique et Planetologie
local.contributor.affiliationChaplin, W. J., Aarhus University
local.contributor.affiliationCunha, M S, Universidade do Porto
local.contributor.affiliationWeiss, A, Max-Planck-Institut fur Astrophysik
local.contributor.affiliationAppourchaux, T, Universite Paris XI
local.contributor.affiliationCasagrande, Luca, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidCasagrande, Luca, u5209059
local.description.notesImported from ARIES
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.ariespublicationf5625xPUB3428
local.identifier.citationvolume769
local.identifier.doi10.1088/0004-637X/769/2/141
local.identifier.scopusID2-s2.0-84878100836
local.identifier.thomsonID000319999100057
local.type.statusPublished Version

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