{"paper":{"title":"The cluster ages experiment (CASE). VII. Analysis of two eclipsing binaries in the globular cluster NGC 6362","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Dotter, A. Schwarzenberg-Czerny, I. B. Thompson, J. Kaluzny, M. Rozyczka","submitted_at":"2015-08-20T06:53:14Z","abstract_excerpt":"We use photometric and spectroscopic observations of the detached eclipsing binaries V40 and V41 in the globular cluster NGC 6362 to derive masses, radii, and luminosities of the component stars. The orbital periods of these systems are 5.30 and 17.89 d, respectively. The measured masses of the primary and secondary components ($M_p$, $M_s$) are (0.8337$\\pm$0.0063, 0.7947$\\pm$0.0048) M$_\\odot$ for V40 and (0.8215$\\pm$0.0058, 0.7280$\\pm$0.0047) M$_\\odot$ for V41. The measured radii ($R_p$, $R_s$) are (1.3253$\\pm$0.0075, 0.997$\\pm$0.013) R$_\\odot$ for V40 and (1.0739$\\pm$0.0048, 0.7307$\\pm$0.004"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1508.04894","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"}