{"paper":{"title":"Study of Eclipsing Binary and Multiple Systems in OB Associations IV: Cas OB6 Member DN Cas","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"H. Bakis, S. Bilir, V. Bakis, Z. Eker","submitted_at":"2016-08-01T14:48:20Z","abstract_excerpt":"An early-type, massive, short-period ($P_{\\rm orb}=2^{\\rm d}.310951$) eclipsing spectroscopic binary DN Cas has been re-visited with new spectral and photometric data. The masses and radii of the components have been obtained as $M_1=19.04\\pm0.07 M_\\odot$, $M_2=13.73\\pm 0.05M_\\odot$ and $R_1=7.22\\pm0.06 R_\\odot$, $R_2=5.79\\pm0.06R_\\odot$, respectively. Both components present synchronous rotation ($V_{\\rm rot1}=160\\,$km s$^{-1}$, $V_{\\rm rot2}=130\\,$km s$^{-1}$) with their orbit. Orbital period analysis yielded a physically bound additional component in the system with a minimum mass of $M_3=0"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1608.00456","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"}