{"paper":{"title":"The Fraction of Stars That Form in Clusters in Different Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alexander J. Mulia, Bradley C. Whitmore, Rupali Chandar, S. Michael Fall","submitted_at":"2018-06-29T17:04:57Z","abstract_excerpt":"We estimate the fraction of stars that form in compact clusters (bound and unbound), Gamma_F, in a diverse sample of eight star-forming galaxies, including two irregulars, two dwarf starbursts, two spirals, and two mergers. The average value for our sample is Gamma_F ~ 24 +/- 9%. We also calculate the fraction of stars in clusters that survive to ages between t1 and t2, denoted by Gamma_S(t1,t2), and find Gamma_S(10,100)=4.6 +/- 2.5% and Gamma_S(100,400)=2.4 +/- 1.1 %, significantly lower than Gamma_F for the same galaxies. We do not find any systematic trends in Gamma_F or Gamma_S with the st"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.11537","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"}