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- W2242758323 endingPage "71" @default.
- W2242758323 startingPage "71" @default.
- W2242758323 abstract "We employ high-resolution cosmological zoom-in simulations focusing on a high-sigma peak and an average cosmological field at z ∼ 6–12 in order to investigate the influence of environment and baryonic feedback on galaxy evolution in the reionization epoch. Strong feedback, e.g., galactic winds, caused by elevated star formation rates (SFRs) is expected to play an important role in this evolution. We compare different outflow prescriptions: (i) constant wind velocity (CW), (ii) variable wind scaling with galaxy properties (VW), and (iii) no outflows (NW). The overdensity leads to accelerated evolution of dark matter and baryonic structures, absent from the normal region, and to shallow galaxy stellar mass functions at the low-mass end. Although CW shows little dependence on the environment, the more physically motivated VW model does exhibit this effect. In addition, VW can reproduce the observed specific SFR (sSFR) and the sSFR–stellar mass relation, which CW and NW fail to satisfy simultaneously. Winds also differ substantially in affecting the state of the intergalactic medium (IGM). The difference lies in the volume-filling factor of hot, high-metallicity gas, which is near unity for CW, while such gas remains confined in massive filaments for VW, and locked up in galaxies for NW. Such gas is nearly absent from the normal region. Although all wind models suffer from deficiencies, the VW model seems to be promising in correlating the outflow properties with those of host galaxies. Further constraints on the state of the IGM at high z are needed to separate different wind models." @default.
- W2242758323 created "2016-06-24" @default.
- W2242758323 creator A5035757328 @default.
- W2242758323 creator A5035867472 @default.
- W2242758323 creator A5059002470 @default.
- W2242758323 creator A5073553250 @default.
- W2242758323 date "2016-09-23" @default.
- W2242758323 modified "2023-09-23" @default.
- W2242758323 title "THE BARYON CYCLE AT HIGH REDSHIFTS: EFFECTS OF GALACTIC WINDS ON GALAXY EVOLUTION IN OVERDENSE AND AVERAGE REGIONS" @default.
- W2242758323 cites W1485788799 @default.
- W2242758323 cites W1534735367 @default.
- W2242758323 cites W1796382164 @default.
- W2242758323 cites W1821343735 @default.
- W2242758323 cites W1821429365 @default.
- W2242758323 cites W1843369788 @default.
- W2242758323 cites W1865796440 @default.
- W2242758323 cites W1867185486 @default.
- W2242758323 cites W1891417619 @default.
- W2242758323 cites W1964280853 @default.
- W2242758323 cites W1964786277 @default.
- W2242758323 cites W1965485119 @default.
- W2242758323 cites W1967407002 @default.
- W2242758323 cites W1969717379 @default.
- W2242758323 cites W1970337192 @default.
- W2242758323 cites W1971602535 @default.
- W2242758323 cites W1971999183 @default.
- W2242758323 cites W1977066125 @default.
- W2242758323 cites W1984607950 @default.
- W2242758323 cites W1987635305 @default.
- W2242758323 cites W1996116122 @default.
- W2242758323 cites W2000265182 @default.
- W2242758323 cites W2001085255 @default.
- W2242758323 cites W2001298730 @default.
- W2242758323 cites W2004310296 @default.
- W2242758323 cites W2008429960 @default.
- W2242758323 cites W2012220297 @default.
- W2242758323 cites W2012886609 @default.
- W2242758323 cites W2013922472 @default.
- W2242758323 cites W2016966639 @default.
- W2242758323 cites W2018539983 @default.
- W2242758323 cites W2019464401 @default.
- W2242758323 cites W2020324400 @default.
- W2242758323 cites W2024931169 @default.
- W2242758323 cites W2034241894 @default.
- W2242758323 cites W2035932765 @default.
- W2242758323 cites W2037526471 @default.
- W2242758323 cites W2037878575 @default.
- W2242758323 cites W2039011228 @default.
- W2242758323 cites W2042482145 @default.
- W2242758323 cites W2046149262 @default.
- W2242758323 cites W2048017362 @default.
- W2242758323 cites W2048744865 @default.
- W2242758323 cites W2048828609 @default.
- W2242758323 cites W2052315062 @default.
- W2242758323 cites W2056409994 @default.
- W2242758323 cites W2058210847 @default.
- W2242758323 cites W2064662554 @default.
- W2242758323 cites W2066744800 @default.
- W2242758323 cites W2067857092 @default.
- W2242758323 cites W2072602795 @default.
- W2242758323 cites W2074252854 @default.
- W2242758323 cites W2080028832 @default.
- W2242758323 cites W2091161890 @default.
- W2242758323 cites W2093419164 @default.
- W2242758323 cites W2096768907 @default.
- W2242758323 cites W2097995542 @default.
- W2242758323 cites W2100514692 @default.
- W2242758323 cites W2101568531 @default.
- W2242758323 cites W2111596254 @default.
- W2242758323 cites W2113723684 @default.
- W2242758323 cites W2114561384 @default.
- W2242758323 cites W2117323006 @default.
- W2242758323 cites W2119131940 @default.
- W2242758323 cites W2120523711 @default.
- W2242758323 cites W2120699388 @default.
- W2242758323 cites W2123464975 @default.
- W2242758323 cites W2128808878 @default.
- W2242758323 cites W2130530521 @default.
- W2242758323 cites W2134712793 @default.
- W2242758323 cites W2136211443 @default.
- W2242758323 cites W2136696603 @default.
- W2242758323 cites W2136969532 @default.
- W2242758323 cites W2147344503 @default.
- W2242758323 cites W2153120512 @default.
- W2242758323 cites W2156621121 @default.
- W2242758323 cites W2162466104 @default.
- W2242758323 cites W2204815181 @default.
- W2242758323 cites W2325917856 @default.
- W2242758323 cites W2953228579 @default.
- W2242758323 cites W2996196020 @default.
- W2242758323 cites W3037641373 @default.
- W2242758323 cites W3098183261 @default.
- W2242758323 cites W3098221464 @default.
- W2242758323 cites W3098935255 @default.
- W2242758323 cites W3099105840 @default.
- W2242758323 cites W3099416141 @default.
- W2242758323 cites W3099762132 @default.
- W2242758323 cites W3099901154 @default.