{"paper":{"title":"A census of dense cores in the Taurus L1495 cloud from the Herschel Gould Belt Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"A. Men'shchikov, A. Roy, D. Elia, D. Ward-Thompson, D. W. Bresnahan, F. Motte, G. J. White, J. Di Francesco, J. M. Kirk, K. A. Marsh, L. Spinoglio, M. Benedettini, M. J. Griffin, N. Peretto, N. Schneider, Ph. Andre, P. Palmeirim, S. Pezzuto, S. Sadavoy, V. Konyves","submitted_at":"2016-02-09T19:58:56Z","abstract_excerpt":"We present a catalogue of dense cores in a $\\sim 4^\\circ\\times2^\\circ$ field of the Taurus star-forming region, inclusive of the L1495 cloud, derived from Herschel SPIRE and PACS observations in the 70 $\\mu$m, 160 $\\mu$m, 250 $\\mu$m, 350 $\\mu$m, and 500 $\\mu$m continuum bands. Estimates of mean dust temperature and total mass are derived using modified blackbody fits to the spectral energy distributions. We detect 525 starless cores of which $\\sim10$-20% are gravitationally bound and therefore presumably prestellar. Our census of unbound objects is $\\sim85$% complete for $M>0.015\\,M_\\odot$ in "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.03143","kind":"arxiv","version":3},"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"}