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dc.contributorDepartment of Physics, Astronomy and Materials Science, Missouri StateUniversity, United States of America
dc.contributorDepartment of Physics, Astronomy and Materials Science, Missouri StateUniversity, United States of America; Suhora Observatory and Krakow Pedagogical University,Krakow, Poland
dc.contributorNordic Optical Telescope,Santa Cruz de Tenerife, Spain
dc.contributorArmagh Observatory and Planetarium,Armagh, Ireland
dc.contributor.authorReed, Michael D.
dc.contributor.authorBaran, Andrzej S.
dc.contributor.authorTelting, John H.
dc.contributor.authorØstensen, Roy H.
dc.contributor.authorJeffery, Christopher S.
dc.contributor.authorKern, Joshua W.
dc.contributor.authorKetzer, Laura
dc.contributor.authorCrooke, John
dc.contributor.authorSlayton, A.
dc.date.accessioned2024-07-24T13:27:32Z
dc.date.available2024-07-24T13:27:32Z
dc.date.issued2018-07-01T00:00:00Z
dc.identifier.doi10.1515/astro-2018-0015
dc.identifier.other2018OAst...27..157R
dc.identifier.other10.1515/astro-2018-0015
dc.identifier.other-
dc.identifier.urihttp://hdl.handle.net/20.500.14302/2068
dc.description.abstractThis paper reviews recent seismic findings from Kepler and K2 data. Using three years of short cadence Kepler (K1) data, it is possible to examine time evolution of pulsations in an unprecedented way. While K2 observations are shorter, only three months, they are important as they are finding more sdBV stars than K1 did. Most importantly, K2 is discovering more p-mode pulsators with coverage not possible to get from the ground.
dc.publisherOpen Astronomy
dc.titleA review of seismic observations of Kepler and K2-Observed sdBV stars
dc.typearticle
dc.source.journalOAst
dc.source.journalOAst...27
dc.source.volume27
refterms.dateFOA2024-07-24T13:27:32Z
dc.identifier.bibcode2018OAst...27..157R


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