{"paper":{"title":"Stellar Physics with High-Resolution UV Spectropolarimetry","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.SR","authors_text":"Agnes L\\`ebre, Alex de Koter, Aline Vidotto, Ana I G\\'omez de Castro, Antoine Strugarek, Artemio Herrero, Beate Stelzer, Chris Evans, Claude Catala, Conny Aerts, Coralie Neiner, Corinne Charbonnel, Gaitee Hussain, Georges Meynet, Jean-Claude Bouret, Ji\\v{r}\\'i\\K{r}ti\\v{c}ka, Jorick S Vink, Julien Morin, Lex Kaper, Luca Fossati, Michaela Kraus, Miriam Garcia, Oleg Kochukhov, Pascal Petit, Renada Konstantinova-Antova, Sami Solanki, Stefano Bagnulo, Steve Shore, Theresa Lueftinger","submitted_at":"2019-08-05T10:14:24Z","abstract_excerpt":"Current burning issues in stellar physics, for both hot and cool stars, concern their magnetism. In hot stars, stable magnetic fields of fossil origin impact their stellar structure and circumstellar environment, with a likely major role in stellar evolution. However, this role is complex and thus poorly understood as of today. It needs to be quantified with high-resolution UV spectropolarimetric measurements. In cool stars, UV spectropolarimetry would provide access to the structure and magnetic field of the very dynamic upper stellar atmosphere, providing key data for new progress to be made"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1908.01545","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1908.01545/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}