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Authordc.contributor.authorJackman, James A. G. 
Authordc.contributor.authorWheatley, Peter J. 
Authordc.contributor.authorActon, Jack S. 
Authordc.contributor.authorAnderson, David R. 
Authordc.contributor.authorBelardi, Claudia 
Authordc.contributor.authorBurleigh, Matthew R. 
Authordc.contributor.authorCasewell, Sarah L. 
Authordc.contributor.authorEigmüller, Philipp 
Authordc.contributor.authorGill, Samuel 
Authordc.contributor.authorGillen, Edward 
Authordc.contributor.authorGoad, Michael R. 
Authordc.contributor.authorGrange, Andrew 
Authordc.contributor.authorHodgkin, Simon T. 
Authordc.contributor.authorJenkins, James 
Authordc.contributor.authorMcCormac, James 
Authordc.contributor.authorMoyano, Maximiliano 
Authordc.contributor.authorQueloz, Didier 
Authordc.contributor.authorRaynard, Liam 
Authordc.contributor.authorTilbrook, Rosanna H. 
Authordc.contributor.authorWatson, Christopher A. 
Authordc.contributor.authorWest, Richard G. 
Admission datedc.date.accessioned2021-03-10T14:19:10Z
Available datedc.date.available2021-03-10T14:19:10Z
Publication datedc.date.issued2020
Cita de ítemdc.identifier.citationMonthly Notices of the Royal Astronomical Society 497(1):809-817es_ES
Identifierdc.identifier.other10.1093/mnras/staa1971
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/178633
Abstractdc.description.abstractWe present the detection of high-energy white-light flares from pre-main-sequence stars associated with the Orion Complex, observed as part of the Next Generation Transit Survey (NGTS). With energies up to 5.2 x 10(35) erg these flares are some of the most energetic white-light flare events seen to date. We have used the NGTS observations of flaring and non-flaring stars to measure the average flare occurrence rate for 4 Myr M0-M3 stars. We have also combined our results with those from previous studies to predict average rates for flares above 1 x 10(35) erg for early M stars in nearby young associations.es_ES
Patrocinadordc.description.sponsorshipUniversity of Warwick University of Leicester Queen's University Belfast University of Geneva Deutsches Zentrum fur Luft-und Raumfahrt e.V. (DLR; under the 'Grossinvestition GI-NGTS') University of Cambridge UK Research & Innovation (UKRI) Science & Technology Facilities Council (STFC) ST/M001962/1 UK Research & Innovation (UKRI) Science & Technology Facilities Council (STFC) 1763096 UK Research & Innovation (UKRI) Science & Technology Facilities Council (STFC) ST/P000495/1 David and Claudia Harding Foundation National Aeronautics & Space Administration (NASA) National Science Foundation (NSF)es_ES
Lenguagedc.language.isoenes_ES
Publisherdc.publisherOxford University Presses_ES
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Sourcedc.sourceMonthly Notices of the Royal Astronomical Societyes_ES
Keywordsdc.subjectStars: flarees_ES
Keywordsdc.subjectStars: pre-main-sequencees_ES
Keywordsdc.subjectStars: low-masses_ES
Títulodc.titleNGTS clusters survey - II. White-light ares from the youngest stars in Oriones_ES
Document typedc.typeArtículo de revistaes_ES
dcterms.accessRightsdcterms.accessRightsAcceso Abierto
Catalogueruchile.catalogadorctces_ES
Indexationuchile.indexArtículo de publicación ISI
Indexationuchile.indexArtículo de publicación SCOPUS


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Attribution-NonCommercial-NoDerivs 3.0 Chile
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile