{"paper":{"title":"The Effect of Star Formation on the Far-Infrared--Radio Correlation within Galaxies","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B. Buckalew, B.T. Draine, C.W. Engelbracht, D.A. Dale, D. Calzetti, E.J. Murphy, F. Walter, G. Helou, G.J. Bendo, H. Roussel, J.D.P. Kenney, J.D.T. Smith, Jr., L. Armus, M.D. Thornley, R. Braun, R.C. Kennicutt","submitted_at":"2006-09-26T20:37:01Z","abstract_excerpt":"Using data obtained for twelve galaxies as part of the {\\it Spitzer} Infrared Nearby Galaxies Survey (SINGS) and the Westerbork Synthesis Radio Telescope (WSRT)-SINGS radio continuum survey, we study how star formation activity affects the far-infrared (FIR)--radio correlation {\\it within} galaxies by testing a phenomenological model, which describes the radio image as a smeared version of the FIR image. The physical basis of this description is that cosmic-ray (CR) electrons will diffuse measurably farther than the mean free path of dust-heating photons before decaying by synchrotron radiatio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0609724","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"}