{"paper":{"title":"Seismic modelling of early B-type pulsators observed by BRITE: I. $\\theta$ Ophiuchi","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Adam Popowicz, Alexey Pamyatnykh, Andrzej Pigulski, Anthony F.J. Moffat, Gerald Handler, Gregg Wade, Herbert Pablo, Jadwiga Daszy\\'nska-Daszkiewicz, Konstanze Zwintz, Przemys{\\l}aw Walczak, Werner W. Weiss","submitted_at":"2019-03-11T11:38:44Z","abstract_excerpt":"We analyse time-series observations from the BRITE-Constellation of the well known $\\beta$ Cephei type star $\\theta$ Ophiuchi. Seven previously known frequencies were confirmed and nineteen new frequency peaks were detected. In particular, high-order g modes, typical for the SPB (Slowly Pulsating B-type star) pulsators, are uncovered. These low-frequency modes are also obtained from the 7-year SMEI light curve. If g modes are associated with the primary component of $\\theta$ Oph, then our discovery allows, as in the case of other hybrid pulsators, to infer more comprehensive information on the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1903.04224","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":""},"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"}