{ "id": "2406.16631", "version": "v1", "published": "2024-06-24T13:26:10.000Z", "updated": "2024-06-24T13:26:10.000Z", "title": "Luminosity Evolution of the Hot Gas in Normal Galaxies from the Near Universe to z=0.5", "authors": [ "Dong-Woo Kim", "Giuseppina Fabbiano" ], "comment": "24 pages, 14 figures, submitted to ApJ", "categories": [ "astro-ph.GA", "astro-ph.HE" ], "abstract": "We explore the evolution of the ~107 degree hot gas in normal galaxies out to redshift = 0.5 (lookback time = 5 Gyr), using X-ray luminosity functions (XLF) built from a sample of 575 normal galaxies with z < 0.6 detected in five high galactic latitude Chandra wide-field surveys. After estimating the emission due to the hot gas component (reducing the sample to ~400 galaxies), we compared the XLF in three redshift bins (z = 0.1, 0.3, and 0.5), finding increases in the number of galaxies per unit co-moving volume from z = 0.1 to 0.3 and then from z = 0.3 to 0.5. These XLF changes suggest a significant (~5s) X-ray luminosity evolution of the hot gas, with LX,GAS decreasing by a factor of 6-10 in the last 5 Gyr (from z = 0.5 to 0.1). The relative abundance of LX,GAS~1041 erg s-1 galaxies at higher z, suggests that high z, moderate LX,GAS galaxies may be the optimal target to solve the missing baryon problem. In early-type galaxies, this observational trend is qualitatively consistent with (but larger than) the expected time-dependent mass-loss rate in cooling flow models without AGN feedback. In late-type galaxies, the observational trend is also qualitatively consistent with (but larger than) the effect of the z-dependent SFR.", "revisions": [ { "version": "v1", "updated": "2024-06-24T13:26:10.000Z" } ], "analyses": { "keywords": [ "normal galaxies", "luminosity evolution", "galactic latitude chandra wide-field surveys", "high galactic latitude chandra wide-field", "x-ray luminosity" ], "note": { "typesetting": "TeX", "pages": 24, "language": "en", "license": "arXiv", "status": "editable" } } }