{ "id": "1009.6005", "version": "v1", "published": "2010-09-29T21:09:50.000Z", "updated": "2010-09-29T21:09:50.000Z", "title": "The Effects of X-Ray and UV Background Radiation on the Low-Mass Slope of the Galaxy Mass Function", "authors": [ "D. C. Hambrick", "J. P. Ostriker", "P. H. Johansson", "T. Naab" ], "comment": "9 pages, 4 figures in mn2e style; submitted to MNRAS", "categories": [ "astro-ph.GA", "astro-ph.CO" ], "abstract": "Even though the dark-matter power spectrum in the absence of biasing predicts a number density of halos n(M) ~ M^-2 (i.e. a Schechter alpha value of -2) at the low-mass end (M < 10^10 M_solar), hydrodynamic simulations have typically produced values for stellar systems in good agreement with the observed value alpha ~ -1. We explain this with a simple physical argument and show that an efficient external gas-heating mechanism (such as the UV background included in all hydro codes) will produce a critical halo mass below which halos cannot retain their gas and form stars. We test this conclusion with GADGET-2-based simulations using various UV backgrounds, and for the first time we also investigate the effect of an X-ray background. We show that at the present epoch alpha is depends primarily on the mean gas temperature at the star-formation epoch for low-mass systems (z <~ 3): with no background we find alpha ~ -1.5, with UV only alpha ~ -1.0, and with UV and X-rays alpha ~ -0.75. We find the critical final halo mass for star formation to be ~4x10^8 M_solar with a UV background and ~7x10^8 M_solar with UV and X-rays.", "revisions": [ { "version": "v1", "updated": "2010-09-29T21:09:50.000Z" } ], "analyses": { "keywords": [ "galaxy mass function", "uv background radiation", "low-mass slope", "halo mass", "efficient external gas-heating mechanism" ], "tags": [ "journal article" ], "publication": { "doi": "10.1111/j.1365-2966.2011.18312.x", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2011, "month": "Jun", "volume": 413, "number": 4, "pages": 2421 }, "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable", "inspire": 871314, "adsabs": "2011MNRAS.413.2421H" } } }