{"paper":{"title":"The complex gas kinematics in the nucleus of the Seyfert 2 galaxy NGC 1386: rotation, outflows and inflows","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Allan Schnorr-Muller, Andrew Robinson, Davide Lena, Guilherme S. Couto, Lucas Shadler, Neil M. Nagar, Rogemar A. Riffel, Thaisa Storchi-Bergmann, Trent Seelig","submitted_at":"2015-04-20T15:41:53Z","abstract_excerpt":"We present optical integral field spectroscopy of the circum-nuclear gas of the Seyfert 2 galaxy NGC 1386. The data cover the central 7$^{\\prime\\prime} \\times 9^{\\prime\\prime}$ (530 $\\times$ 680 pc) at a spatial resolution of 0.9\" (68 pc), and the spectral range 5700-7000 \\AA\\ at a resolution of 66 km s$^{-1}$. The line emission is dominated by a bright central component, with two lobes extending $\\approx$ 3$^{\\prime\\prime}$ north and south of the nucleus. We identify three main kinematic components. The first has low velocity dispersion ($\\bar \\sigma \\approx $ 90 km s$^{-1}$), extends over th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1504.05089","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"}