{ "id": "1707.03879", "version": "v1", "published": "2017-07-12T19:21:24.000Z", "updated": "2017-07-12T19:21:24.000Z", "title": "The SAMI Galaxy Survey: Disk-halo interactions in radio-selected star-forming galaxies", "authors": [ "S. K. Leslie", "J. J. Bryant", "I. -T. Ho", "E. M. Sadler", "A. M. Medling", "B. Groves", "L. J. Kewley", "J. Bland-Hawthorn", "S. M. Croom", "O. I. Wong", "S. Brough", "E. Tescari", "S. M. Sweet", "R. Sharp", "A. W. Green", "A. R. López-Sánchez", "J. T. Allen", "L. M. R. Fogarty", "M. Goodwin", "J. S. Lawrence", "I. S. Konstantopoulos", "M. S. Owers", "S. N. Richards" ], "comment": "16 pages, 5 figures. Published in MNRAS July 2017", "doi": "10.1093/mnras/stx1673", "categories": [ "astro-ph.GA" ], "abstract": "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 the strongest wind signatures have extended radio morphologies. Our results form a baseline for understanding the driving mechanisms of galactic winds.", "revisions": [ { "version": "v1", "updated": "2017-07-12T19:21:24.000Z" } ], "analyses": { "keywords": [ "sami galaxy survey", "radio-selected star-forming galaxies", "disk-halo interactions", "sydney-aao multi-object integral-field spectrograph", "galactic winds" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 16, "language": "en", "license": "arXiv", "status": "editable" } } }