{"paper":{"title":"Planck Cold Clumps in the $\\lambda$ Orionis complex. II. Environmental effects on core formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"Archana Soam, Chang Won Lee, David Eden, Di Li, Gary Fuller, Glenn J. White, Gwanjeong Kim, Hee-Weon Yi, Hong-Li Liu, H.-Y. B. Liu, I. Ristorcelli, James Di Francesco, Jeong-Eun Lee, Kee-Tae Kim, Ken'ichi Tatematsu, Ke Wang, L. V. Toth, Mark G. Rawlings, Mark Thompson, Mika Juvela, Minho Choi, Neal J. Evans II, N. Hirano, Patrick M. Koch, Patrico Sanhueza, Sheng-Yuan Liu, Sung-Ju Kang, Tie Liu, Yao-Lun Yang, Yuefang Wu","submitted_at":"2018-05-15T12:51:17Z","abstract_excerpt":"Based on the 850 $\\mu$m dust continuum data from SCUBA-2 at James Clerk Maxwell Telescope (JCMT), we compare overall properties of Planck Galactic Cold Clumps (PGCCs) in the $\\lambda$ Orionis cloud to those of PGCCs in the Orion A and B clouds. The Orion A and B clouds are well known active star-forming regions, while the $\\lambda$ Orionis cloud has a different environment as a consequence of the interaction with a prominent OB association and a giant Hii region. PGCCs in the $\\lambda$ Orionis cloud have higher dust temperatures ($Td=16.13\\pm0.15$ K) and lower values of dust emissivity spectra"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1805.05738","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"}