{"paper":{"title":"ALMA-IMF XVI: Mass-averaged temperature of cores and protostellar luminosities in the ALMA-IMF protoclusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Ginsburg, A. Gusdorf, A. Koley, A. Men'shchikov, A. M. Stutz, B. Lefloch, D. D\\'iaz-Gonz\\'alez, E. Moraux, F. Herpin, F. Louvet, F. Motte, F. Olguin, H.-L. Liu, H.-R. V. Chen, J. Salinas, L. Bronfman, M. Armante, M. Bonfand, M. Fern\\'andez-L\\'opez, M. Valeille-Manet, N. A. Sandoval-Garrido, N. Brouillet, N. Cunningham, N. Kessler, N. Le Nestour, P. Dell'Ova, P. Didelon, P. Sanhueza, Q. Nguyen Luong, R. Galv\\'an-Madrid, R. H. \\'Alvarez-Guti\\'errez, R. Veyry, S. Bontemps, T. Csengeri, T. Nony, T. Yoo, Y. Pouteau","submitted_at":"2024-12-02T22:30:38Z","abstract_excerpt":"ALMA-IMF imaged 15 massive protoclusters down to a resolution of of 2 kau scales, identifying about 1000 star-forming cores. The mass and luminosity of these cores, which are fundamental physical characteristics, are difficult to determine, a problem greatly exacerbated at the distances >2 kpc of ALMA-IMF protoclusters. We combined new datasets and radiative transfer modeling to characterize these cores. We estimated their mass-averaged temperature and the masses these estimates imply. For 1/6 of the sample, we measured the bolometric luminosities, implementing deblending corrections when nece"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.02011","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2412.02011/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"}