Poster Open Access
Ilin, Ekaterina;
Poppenhäger, Katja;
Schmidt, Sarah J.;
Järvinen, Silva P.;
Newton, Elisabeth R.;
Alvarado-Gómez, Julián D.;
Pineda, J. Sebastian;
Davenport, James R. A.;
Oshagh, Mahmoudreza;
Ilyin, Ilya
<?xml version='1.0' encoding='utf-8'?> <oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"> <dc:creator>Ilin, Ekaterina</dc:creator> <dc:creator>Poppenhäger, Katja</dc:creator> <dc:creator>Schmidt, Sarah J.</dc:creator> <dc:creator>Järvinen, Silva P.</dc:creator> <dc:creator>Newton, Elisabeth R.</dc:creator> <dc:creator>Alvarado-Gómez, Julián D.</dc:creator> <dc:creator>Pineda, J. Sebastian</dc:creator> <dc:creator>Davenport, James R. A.</dc:creator> <dc:creator>Oshagh, Mahmoudreza</dc:creator> <dc:creator>Ilyin, Ilya</dc:creator> <dc:date>2021-10-10</dc:date> <dc:description>In a systematic analysis of late M dwarfs observed with TESS, we detected four stars with giant flares that were modulated in brightness by the stars' rapid rotation. Using the shape of the modulated curve we could localize these flares between 55° and 81° latitude on the stellar surface, far higher than typical solar flare latitudes.</dc:description> <dc:identifier>https://zenodo.org/record/5559296</dc:identifier> <dc:identifier>10.5281/zenodo.5559296</dc:identifier> <dc:identifier>oai:zenodo.org:5559296</dc:identifier> <dc:relation>doi:10.5281/zenodo.5559295</dc:relation> <dc:relation>url:https://zenodo.org/communities/plato2021</dc:relation> <dc:rights>info:eu-repo/semantics/openAccess</dc:rights> <dc:rights>https://creativecommons.org/licenses/by/4.0/legalcode</dc:rights> <dc:source>Monthly Notices of the Royal Astronomical Society 507(2) 1723-1745</dc:source> <dc:subject>stars</dc:subject> <dc:subject>fully convective stars</dc:subject> <dc:subject>flares</dc:subject> <dc:subject>habitability</dc:subject> <dc:subject>stellar activity</dc:subject> <dc:subject>stellar magnetic fields</dc:subject> <dc:subject>TESS</dc:subject> <dc:title>Giant white-light flares on fully convective stars occur at high latitudes</dc:title> <dc:type>info:eu-repo/semantics/conferencePoster</dc:type> <dc:type>poster</dc:type> </oai_dc:dc>
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