{"paper":{"title":"Novae II. Model, multi-band outburst, bipolar ejecta, accretion disk, relativistic electrons, etc","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"Nimisha Kantharia (National Centre for Radio Astrophysics, Pune), Tata Institute of Fundamental Research","submitted_at":"2017-09-27T09:13:06Z","abstract_excerpt":"The study of novae is continued and a self-consistent updated physical model for classical/recurrent novae derived from multi-wavelength observations is presented. In particular, observations of novae support the origin of the optical continuous emission in the outburst ejecta, mass-based segregation and clump formation in the ejecta, origin of the Orion, diffuse enhanced lines and dust in the clumps, prompt Fe II line formation in swept-up material, energising of electrons to relativistic velocities by the explosion and the existence of a large cool envelope around the accreting white dwarf i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.09400","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"}