1. Repositório Aberto da Universidade do Porto
  2. FCUP - Faculdade de Ciências
  3. FCUP - Artigo em Revista Científica Internacional
Please use this identifier to cite or link to this item: https://hdl.handle.net/10216/94642
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dc.creatorChaplin, WJ
dc.creatorAppourchaux, T
dc.creatorElsworth, Y
dc.creatorGarcia, RA
dc.creatorHoudek, G
dc.creatorKaroff, C
dc.creatorMetcalfe, TS
dc.creatorMolenda Zakowicz, J
dc.creatorMonteiro, MJPFG
dc.creatorThompson, MJ
dc.creatorBrown, TM
dc.creatorChristensen Dalsgaard, J
dc.creatorGilliland, RL
dc.creatorKjeldsen, H
dc.creatorBorucki, WJ
dc.creatorKoch, D
dc.creatorJenkins, JM
dc.creatorBallot, J
dc.creatorBasu, S
dc.creatorBazot, M
dc.creatorBedding, TR
dc.creatorBenomar, O
dc.creatorBonanno, A
dc.creatorBrandao, IM
dc.creatorBruntt, H
dc.creatorCampante, TL
dc.creatorCreevey, OL
dc.creatorDi Mauro, MP
dc.creatorDogan, G
dc.creatorDreizler, S
dc.creatorEggenberger, P
dc.creatorEsch, L
dc.creatorFletcher, ST
dc.creatorFrandsen, S
dc.creatorGai, N
dc.creatorGaulme, P
dc.creatorHandberg, R
dc.creatorHekker, S
dc.creatorHowe, R
dc.creatorHuber, D
dc.creatorKorzennik, SG
dc.creatorLebrun, JC
dc.creatorLeccia, S
dc.creatorMartic, M
dc.creatorMathur, S
dc.creatorMosser, B
dc.creatorNew, R
dc.creatorO Quirion
dc.creatorRegulo, C
dc.creatorRoxburgh, IW
dc.creatorSalabert, D
dc.creatorSchou, J
dc.creatorSousa, SG
dc.creatorStello, D
dc.creatorVerner, GA
dc.creatorArentoft, T
dc.creatorBarban, C
dc.creatorBelkacem, K
dc.creatorBenatti, S
dc.creatorBiazzo, K
dc.creatorBoumier, P
dc.creatorBradley, PA
dc.creatorM Broomhall
dc.creatorBuzasi, DL
dc.creatorClaudi, RU
dc.creatorCunha, MS
dc.creatorD'Antona, F
dc.creatorDeheuvels, S
dc.creatorDerekas, A
dc.creatorGarcia Hernandez, AG
dc.creatorGiampapa, MS
dc.creatorGoupil, MJ
dc.creatorGruberbauer, M
dc.creatorGuzik, JA
dc.creatorHale, SJ
dc.creatorIreland, MJ
dc.creatorKiss, LL
dc.creatorKitiashvili, IN
dc.creatorKolenberg, K
dc.creatorKorhonen, H
dc.creatorKosovichev, AG
dc.creatorKupka, F
dc.creatorLebreton, Y
dc.creatorLeroy, B
dc.creatorG Ludwig
dc.creatorMathis, S
dc.creatorMichel, E
dc.creatorMiglio, A
dc.creatorMontalban, J
dc.creatorMoya, A
dc.creatorNoels, A
dc.creatorNoyes, RW
dc.creatorPalle, PL
dc.creatorPiau, L
dc.creatorPreston, HL
dc.creatorRoca Cortes, TR
dc.creatorRoth, M
dc.creatorSato, KH
dc.creatorSchmitt, J
dc.creatorSerenelli, AM
dc.creatorSilva S Aguirre
dc.creatorStevens, IR
dc.creatorSuarez, JC
dc.creatorSuran, MD
dc.creatorTrampedach, R
dc.creatorTurck Chieze, S
dc.creatorUytterhoeven, K
dc.creatorVentura, R
dc.creatorWilson, PA
dc.date.accessioned2022-09-13T14:57:46Z-
dc.date.available2022-09-13T14:57:46Z-
dc.date.issued2010
dc.identifier.issn2041-8205
dc.identifier.othersigarra:48355
dc.identifier.urihttps://hdl.handle.net/10216/94642-
dc.description.abstractWe present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5 days 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.language.isoeng
dc.rightsrestrictedAccess
dc.subjectAstrofísica, Astronomia, Ciências Físicas, Física
dc.subjectAstrophysics, Astronomy, Physical sciences, Physical sciences
dc.titleTHE ASTEROSEISMIC POTENTIAL OF KEPLER: FIRST RESULTS FOR SOLAR-TYPE STARS
dc.typeArtigo em Revista Científica Internacional
dc.contributor.uportoFaculdade de Ciências
dc.identifier.doi10.1088/2041-8205/713/2/l169
dc.identifier.authenticusP-003-7EE
dc.subject.fosCiências exactas e naturais::Física
dc.subject.fosNatural sciences::Physical sciences
Appears in Collections:FCUP - Artigo em Revista Científica Internacional

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