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The asteroseismic potential of kepler: First results for solar-type stars

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dc.contributor.authorChaplin, W Jen_AU
dc.contributor.authorAppourchaux, Ten_AU
dc.contributor.authorElsworth, Yen_AU
dc.contributor.authorGarcia, R Aen_AU
dc.contributor.authorHoudek, Gen_AU
dc.contributor.authorKaroff, Cen_AU
dc.contributor.authorMetcalfe, T Sen_AU
dc.contributor.authorMolenda-Zakowicz, Jen_AU
dc.contributor.authorMonteiro, M J P F Gen_AU
dc.contributor.authorThompson, M Jen_AU
dc.contributor.authorIreland, Michaelen_AU
dc.date.accessioned2015-12-10T23:23:06Z
dc.date.issued2010
dc.date.updated2016-02-24T09:59:19Z
dc.description.abstractWe present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5days of science operations, reveal high signal-to-noise solar-like oscillation spectra in all three stars: about 20 modes of oscillation may be clearly distinguished in each star. We discuss the appearance of the oscillation spectra, use the frequencies and frequency separations to provide first results on the radii, masses, and ages of the stars, and comment in the light of these results on prospects for inference on other solar-type stars that Kepler will observe.
dc.identifier.issn2041-8205
dc.identifier.urihttp://hdl.handle.net/1885/66806
dc.publisherInstitute of Physics Publishing Ltd.
dc.sourceAstrophysical Journal Letters
dc.subjectKeywords: Stars: interiors; Stars: late-type; Stars: oscillations
dc.titleThe asteroseismic potential of kepler: First results for solar-type stars
dc.typeJournal article
local.bibliographicCitation.issue2 PART 2
local.bibliographicCitation.lastpageL175
local.bibliographicCitation.startpageL169
local.contributor.affiliationChaplin, W J, University of Birmingham
local.contributor.affiliationAppourchaux, T, Universite Paris XI
local.contributor.affiliationElsworth, Y, University of Birmingham
local.contributor.affiliationGarcia, R A, CEA/DSM-CNRS-Universite Paris Diderot
local.contributor.affiliationHoudek, G, University of Vienna
local.contributor.affiliationKaroff, C, University of Birmingham
local.contributor.affiliationMetcalfe, T S, National Center for Atmospheric Research
local.contributor.affiliationMolenda-Zakowicz, J, University of Wrocław
local.contributor.affiliationMonteiro, M J P F G, Universidade do Porto
local.contributor.affiliationThompson, M J, University of Sheffield
local.contributor.affiliationIreland, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidIreland, Michael, u5544212
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationU3488905xPUB1348
local.identifier.citationvolume713
local.identifier.doi10.1088/2041-8205/713/2/L169
local.identifier.scopusID2-s2.0-77950577829
local.type.statusPublished Version

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