1. Repositório Aberto da Universidade do Porto
  2. FCUP - Faculdade de Ciências
  3. FCUP - Artigo em Revista Científica Internacional
Utilize este identificador para referenciar este registo: https://hdl.handle.net/10216/92194
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Campo DCValorIdioma
dc.creatorChaplin, WJ
dc.creatorKjeldsen, H
dc.creatorChristensen Dalsgaard, J
dc.creatorBasu, S
dc.creatorMiglio, A
dc.creatorAppourchaux, T
dc.creatorBedding, TR
dc.creatorElsworth, Y
dc.creatorGarcia, RA
dc.creatorGilliland, RL
dc.creatorGirardi, L
dc.creatorHoudek, G
dc.creatorKaroff, C
dc.creatorKawaler, SD
dc.creatorMetcalfe, TS
dc.creatorMolenda Zakowicz, J
dc.creatorMonteiro, MJPFG
dc.creatorThompson, MJ
dc.creatorVerner, GA
dc.creatorBallot, J
dc.creatorBonanno, A
dc.creatorBrandao, IM
dc.creatorBroomhall, AM
dc.creatorBruntt, H
dc.creatorCampante, TL
dc.creatorCorsaro, E
dc.creatorCreevey, OL
dc.creatorDogan, G
dc.creatorEsch, L
dc.creatorGai, N
dc.creatorGaulme, P
dc.creatorHale, SJ
dc.creatorHandberg, R
dc.creatorHekker, S
dc.creatorHuber, D
dc.creatorJimenez, A
dc.creatorMathur, S
dc.creatorMazumdar, A
dc.creatorMosser, B
dc.creatorNew, R
dc.creatorPinsonneault, MH
dc.creatorPricopi, D
dc.creatorQuirion, PO
dc.creatorRegulo, C
dc.creatorSalabert, D
dc.creatorSerenelli, AM
dc.creatorSilva S Aguirre
dc.creatorSousa, SG
dc.creatorStello, D
dc.creatorStevens, IR
dc.creatorSuran, MD
dc.creatorUytterhoeven, K
dc.creatorWhite, TR
dc.creatorBorucki, WJ
dc.creatorBrown, TM
dc.creatorJenkins, JM
dc.creatorKinemuchi, K
dc.creatorVan Cleve, J
dc.creatorKlaus, TC
dc.date.accessioned2022-09-07T16:06:47Z-
dc.date.available2022-09-07T16:06:47Z-
dc.date.issued2011
dc.identifier.issn0036-8075
dc.identifier.othersigarra:48191
dc.identifier.urihttps://hdl.handle.net/10216/92194-
dc.descriptionIn addition to its search for extrasolar planets, the NASA Kepler mission provides exquisite data on stellar oscillations. We report the detections of oscillations in 500 solar-type stars in the Kepler field of view, an ensemble that is large enough to allow statistical studies of intrinsic stellar properties (such as mass, radius, and age) and to test theories of stellar evolution. We find that the distribution of observed masses of these stars shows intriguing differences to predictions from models of synthetic stellar populations in the Galaxy.
dc.description.abstractIn addition to its search for extrasolar planets, the NASA Kepler mission provides exquisite data on stellar oscillations. We report the detections of oscillations in 500 solar-type stars in the Kepler field of view, an ensemble that is large enough to allow statistical studies of intrinsic stellar properties (such as mass, radius, and age) and to test theories of stellar evolution. We find that the distribution of observed masses of these stars shows intriguing differences to predictions from models of synthetic stellar populations in the Galaxy.
dc.language.isoeng
dc.rightsrestrictedAccess
dc.subjectAstronomia, Física
dc.subjectAstronomy, Physical sciences
dc.titleEnsemble Asteroseismology of Solar-Type Stars with the NASA Kepler Mission
dc.typeArtigo em Revista Científica Internacional
dc.contributor.uportoFaculdade de Ciências
dc.identifier.doi10.1126/science.1201827
dc.identifier.authenticusP-002-SEX
dc.subject.fosCiências exactas e naturais::Física
dc.subject.fosNatural sciences::Physical sciences
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