{"paper":{"title":"A survey for variable young stars with small telescopes: VI -- Analysis of the outbursting Be stars NSW284, Gaia19eyy, and VES263","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Aashini L. Patel, Adam Popowicz, Alex Escartin Perez, Andrzej Malcher, Anna M. Moore, Barry Merrikin, Carys Herbert, David A. Campbell, Dawid Mo\\'zdzierski, Diego Rodriguez, Dirk Froebrich, Francisco C. Sold\\'an Alfaro, Franky Dubois, Franz-Josef Hambsch, George Fleming, Georg Piehler, Heinz-Bernd Eggenstein, Ivan L Walton, Jack Finch, Jerzy Fiolka, Jochen Eisl\\\"offel, Justyn Campbell-White, Kishalay De, Krzysztof Bernacki, Lord Dover, Ludwig Logie, Lynne A. Hillenbrand, Marek Szczepanski, Mario Morales Aimar, Mark Phillips, Matt Hankins, Niall Miller, Pat Devine, Piotr Jozwik-Wabik, Przemys{\\l}aw J. Miko{\\l}ajczyk, Rafael Gonzalez Farf\\'an, Ruhee Kahar, Samantha M. Rolfe, Siegfried Vanaverbeke, Slawomir Lasota, Stephen R.L. Futcher, Steve Rau, Thomas Urtly, Tim Nelson, Tony Travouillon, Tony Vale, Yenal \\\"O\\u{g}men","submitted_at":"2023-02-06T10:53:13Z","abstract_excerpt":"This paper is one in a series reporting results from small telescope observations of variable young stars. Here, we study the repeating outbursts of three likely Be stars based on long-term optical, near-infrared, and mid-infrared photometry for all three objects, along with follow-up spectra for two of the three. The sources are characterised as rare, truly regularly outbursting Be stars. We interpret the photometric data within a framework for modelling light curve morphology, and find that the models correctly predict the burst shapes, including their larger amplitudes and later peaks towar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2302.02696","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/2302.02696/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"}