{ "id": "2004.09873", "version": "v1", "published": "2020-04-21T10:07:24.000Z", "updated": "2020-04-21T10:07:24.000Z", "title": "Sub-galactic scaling relations between X-ray luminosity, star-formation rate, and stellar mass", "authors": [ "Konstantinos Kouroumpatzakis", "Andreas Zezas", "Paul Sell", "Konstantinos Kovlakas", "Paolo Bonfini", "Steven Willner", "Matthew Ashby", "Alexandros Maragkoudakis", "Thomas Jarrett" ], "comment": "19 pages, 13 figures, accepted for publication in MNRAS (2020-04-19)", "doi": "10.1093/mnras/staa1063", "categories": [ "astro-ph.GA" ], "abstract": "X-ray luminosity ($L_X$) originating from high-mass X-ray binaries (HMXBs) is tightly correlated with the host galaxy's star-formation rate (SFR). We explore this connection at sub-galactic scales spanning ${\\sim}$7 dex in SFR and ${\\sim}$8 dex in specific SFR (sSFR). There is good agreement with established relations down to ${\\rm SFR {\\simeq} 10^{-3}\\,M_\\odot \\, yr^{-1}}$, below which an excess of X-ray luminosity emerges. This excess likely arises from low mass X-ray binaries. The intrinsic scatter of the $L_X$-SFR relation is constant, not correlated with SFR. Different star formation indicators scale with $L_X$ in different ways, and we attribute the differences to the effect of star formation history. The SFR derived from H$\\alpha$ shows the tightest correlation with X-ray luminosity because H$\\alpha$ emission probes stellar populations with ages similar to HMXB formation timescales, but the H$\\alpha$-based SFR is reliable only for $\\rm sSFR{>}10^{-12}\\,M_\\odot \\, yr^{-1}/M_\\odot$.", "revisions": [ { "version": "v1", "updated": "2020-04-21T10:07:24.000Z" } ], "analyses": { "keywords": [ "x-ray luminosity", "sub-galactic scaling relations", "stellar mass", "low mass x-ray binaries", "emission probes stellar populations" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 19, "language": "en", "license": "arXiv", "status": "editable" } } }