{"paper":{"title":"Why is there a Dearth of Close-In Planets around Fast-Rotating stars?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Arieh K\\\"onigl, Seth Teitler","submitted_at":"2014-03-24T05:51:38Z","abstract_excerpt":"We propose that the reported dearth of $Kepler$ Objects of Interest (KOIs) with orbital periods $P_{\\rm orb} \\lesssim 2-3\\;$days around stars with rotation periods $P_{\\rm rot} \\lesssim 5-10\\;$days can be attributed to tidal ingestion of close-in planets by their host stars. We show that the planet distribution in this region of the $\\log{P_{\\rm orb}}-\\log{P_{\\rm rot}}$ plane is qualitatively reproduced with a model that incorporates tidal interaction and magnetic braking as well as the dependence on the stellar core--envelope coupling timescale. We demonstrate the consistency of this scenario"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.5860","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"}