{"paper":{"title":"Numerical Simulation of the SVS 13 Micro-Jet and Bow Shock Bubble","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Carl L. Gardner, Jeremiah R. Jones, Klaus W. Hodapp","submitted_at":"2017-06-15T16:34:49Z","abstract_excerpt":"Numerical simulations are performed using the WENO method of the SVS 13 micro-jet and bow shock bubble which reproduce the main features and dynamics of Keck Telescope/OSIRIS velocity-resolved integral field spectrograph data: an expanding cooler bow shock bubble, with the bubble center moving at approximately 50 km/s with a radial expansion velocity of 11 km/s, surrounding the fast hotter jet, which is propagating at 156 km/s. Contact and bow shock waves are visible in the simulations from both the initial short jet pulse which creates the nearly spherical bow shock bubble and from the fast m"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.04955","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"}