{"id":"W2026853476","doi":"10.1051/0004-6361/201014666","title":"From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the<i>Herschel</i>Gould Belt Survey","year":2010,"lang":"en","type":"article","venue":"Astronomy and Astrophysics","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1458,"is_retracted":false,"has_abstract":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; Herzberg Institute of Astrophysics","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Max-Planck-Institut für Astronomie; Science and Technology Facilities Council; Bundesministerium für Verkehr, Innovation und Technologie; Centre National de la Recherche Scientifique; KU Leuven; National Aeronautics and Space Administration; California Institute of Technology; Imperial College London; Centre National d’Etudes Spatiales","keywords":"Protostar; Star formation; Core (optical fiber); Molecular cloud; Initial mass function; Young stellar object; Flare; Circumstellar disk","routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false,"invisible_to_affiliation_only":false},"retraction":null,"screen":null,"machine_scores":{"provisional":true,"baseline":true,"maturity_gate_passed":false,"score_opus":0.01287894295936347,"score_gpt":0.2391222823118036,"score_spread":0.2262433393524401,"validation_status":"score_only:v0-immature-baseline","note":"Baseline scores from an immature model (maturity gate not passed). Scores rank; they never assert a category."}}