{"paper":{"title":"EVLA observations of the nebula around G79.29+0.46","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"1), (2) Universita' di Catania, A. Ingallinera (2, A. Noriega-Crespo (3), C. Agliozzo, California Institute of Technology, Cambridge, C. S. Buemi, C. Trigilio, G. Umana, Italy, Italy (3) Spitzer Science Center, J. L. Hora (4) ((1) INAF-Osservatorio Astrofisico di Catania, MA, Pasadena, P. Leto (1), USA), USA (4) Harvard-Smithsonian Center for Astrophysics","submitted_at":"2011-07-04T16:55:12Z","abstract_excerpt":"We have observed the radio nebula surrounding the Galactic LBV candidate G79.29+0.46 with the EVLA at 6 cm. These new radio observations allow a morphological comparison between the radio emission, which traces the ionized gas component, and the mid-IR emission, a tracer of the dust component. The IRAC (8 \\mu m) and MIPS (24 \\mu m and 70 \\mu m) images have been reprocessed and compared with the EVLA map. We confirm the presence of a second shell at 24 \\mu m and also provide evidence for its detection at 70 \\mu m. The differences between the spatial morphology of the radio and mid-IR maps indic"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1107.0679","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"}