{"paper":{"title":"The SAMI Galaxy Survey: Disk-halo interactions in radio-selected star-forming galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. M. Medling, A. R. L\\'opez-S\\'anchez, A. W. Green, B. Groves, E. M. Sadler, E. Tescari, I.S. Konstantopoulos, I.-T. Ho, J. Bland-Hawthorn, J. J. Bryant, J. S. Lawrence, J. T. Allen, L. J. Kewley, L. M. R. Fogarty, M. Goodwin, M. S. Owers, O. I. Wong, R. Sharp, S. Brough, S. K. Leslie, S. M. Croom, S. M. Sweet, S. N. Richards","submitted_at":"2017-07-12T19:21:24Z","abstract_excerpt":"In this paper, we compare the radio emission at 1.4 GHz with optical outflow signatures of edge-on galaxies. We report observations of six edge-on star-forming galaxies in the Sydney-AAO Multi-object Integral-field spectrograph (SAMI) Galaxy Survey with 1.4 GHz luminosities $> 1\\times10^{21}$ W Hz$^{-1}$. Extended minor axis optical emission is detected with enhanced \\nii/H$\\alpha$ line ratios and velocity dispersions consistent with galactic winds in three of six galaxies. These galaxies may host outflows driven by a combination of thermal and cosmic ray processes. We find that galaxies with "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.03879","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"}