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dc.contributor.authorRaetz, Stefanie
dc.contributor.authorStelzer, Beate
dc.contributor.authorScholz, Alexander
dc.date.accessioned2021-06-24T23:35:46Z
dc.date.available2021-06-24T23:35:46Z
dc.date.issued2020-08-27
dc.identifier.citationRaetz , S , Stelzer , B & Scholz , A 2020 , ' The rotation–activity relation of M dwarfs : from K2 to TESS and PLATO ' , Astronomische Nachrichten , vol. 341 , no. 5 , pp. 519-556 . https://doi.org/10.1002/asna.202013727en
dc.identifier.issn0004-6337
dc.identifier.otherPURE: 268938802
dc.identifier.otherPURE UUID: 9d05cf58-dbd8-45e8-9b0b-48cb8dea84c2
dc.identifier.otherRIS: urn:6723C317AE34892E73CCE01E030AB39C
dc.identifier.otherScopus: 85087218091
dc.identifier.otherWOS: 000563771700007
dc.identifier.urihttp://hdl.handle.net/10023/23419
dc.description.abstractStudies of the rotation–activity relation of late‐type stars are essential to enhance our understanding of stellar dynamos and angular momentum evolution. We study the rotation–activity relation with K2 for M dwarfs, where it is especially poorly understood. We analyzed the light curves of all bright and nearby M dwarfs form the Superblink proper motion catalog that were in the K2 field of view. Using a sample of 430 M dwarfs observed in campaigns C0–C19 in long‐cadence mode, we determined the rotation period and a wealth of activity diagnostics. Our study of the rotation–activity relation based on photometric activity indicators confirmed the previously published abrupt change of the activity level at a rotation period of ∼10 days. Our sample, which is more than three times larger, increases the statistical significance of this finding.
dc.language.isoeng
dc.relation.ispartofAstronomische Nachrichtenen
dc.rightsCopyright © 2020 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim. This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the author created accepted manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1002/asna.202013727.en
dc.subjectStars: late-typeen
dc.subjectStars: activityen
dc.subjectStars: rotationen
dc.subjectStars: flareen
dc.subjectQB Astronomyen
dc.subjectDASen
dc.subject.lccQBen
dc.titleThe rotation–activity relation of M dwarfs : from K2 to TESS and PLATOen
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews.St Andrews Centre for Exoplanet Scienceen
dc.identifier.doihttps://doi.org/10.1002/asna.202013727
dc.description.statusPeer revieweden
dc.identifier.urlhttps://arxiv.org/abs/2005.08688en


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