{"paper":{"title":"The Properties of the Star-Forming Interstellar Medium at z=0.8-2.2 from HiZELS - II: Star-Formation and Clump Scaling Laws in Gas Rich, Turbulent Disks","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"((1) ICC, (2) Leiden, 3), (3) IfA, 4), (4) Antwerp, (5) McGill), David Sobral (2, Durham, Edinburgh, Ian Smail (1), Jim Geach (5), Mark Swinbank (1), Philip Best (3), Tom Theuns (1","submitted_at":"2012-09-06T20:00:26Z","abstract_excerpt":"We present adaptive optics assisted integral field spectroscopy of nine Halpha-selected galaxies at z=0.84--2.23 selected from the HiZELS narrow-band survey. Our observations map the star-formation and kinematics of these representative star-forming galaxies on ~kpc-scales. We demonstrate that within the ISM of these galaxies, the velocity dispersion of the star-forming gas (\\sigma) follows a scaling relation \\sigma\\propto\\Sigma_SFR^(1/n)+constant (where \\Sigma_SFR is the star formation surface density and the constant includes the stellar surface density). Assuming the disks are marginally st"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1209.1396","kind":"arxiv","version":2},"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"}