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- W2897414813 abstract "ABSTRACT We examine the origin of scatter in the relationship between the gas fraction and mass of dark matter haloes hosting present-day ∼L⋆ central galaxies in the EAGLE simulations. The scatter is uncorrelated with the accretion rate of the central galaxy’s black hole (BH), but correlates strongly and negatively with the BH’s mass, implicating differences in the expulsion of gas by active galactic nucleus feedback, throughout the assembly of the halo, as the main cause of scatter. Haloes whose central galaxies host undermassive BHs also tend to retain a higher gas fraction, and exhibit elevated star formation rates (SFRs). Diversity in the mass of central BHs stems primarily from diversity in the dark matter halo binding energy, as these quantities are strongly and positively correlated at fixed halo mass, such that ∼L⋆ galaxies hosted by haloes that are more (less) tightly bound develop central BHs that are more (less) massive than is typical for their halo mass. Variations in the halo gas fraction at fixed halo mass are reflected in both the soft X-ray luminosity and thermal Sunyaev–Zel’dovich flux, suggesting that the prediction of a strong coupling between the properties of galaxies and their halo gas fractions can be tested with measurements of these diagnostics for galaxies with diverse SFRs but similar halo masses." @default.
- W2897414813 created "2018-10-26" @default.
- W2897414813 creator A5007574967 @default.
- W2897414813 creator A5020847721 @default.
- W2897414813 creator A5033973593 @default.
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- W2897414813 creator A5044467709 @default.
- W2897414813 creator A5059148355 @default.
- W2897414813 creator A5084334550 @default.
- W2897414813 date "2019-03-05" @default.
- W2897414813 modified "2023-10-16" @default.
- W2897414813 title "The gas fractions of dark matter haloes hosting simulated ∼L⋆ galaxies are governed by the feedback history of their black holes" @default.
- W2897414813 cites W1735913374 @default.
- W2897414813 cites W1802527253 @default.
- W2897414813 cites W1865574940 @default.
- W2897414813 cites W1883767967 @default.
- W2897414813 cites W1894477963 @default.
- W2897414813 cites W1894826066 @default.
- W2897414813 cites W1921476237 @default.
- W2897414813 cites W1922682040 @default.
- W2897414813 cites W1940538082 @default.
- W2897414813 cites W1943789795 @default.
- W2897414813 cites W1952571495 @default.
- W2897414813 cites W1975549749 @default.
- W2897414813 cites W1975983552 @default.
- W2897414813 cites W1977635644 @default.
- W2897414813 cites W1982655690 @default.
- W2897414813 cites W1990401433 @default.
- W2897414813 cites W2002044265 @default.
- W2897414813 cites W2004591806 @default.
- W2897414813 cites W2006160097 @default.
- W2897414813 cites W2008429960 @default.
- W2897414813 cites W2013979799 @default.
- W2897414813 cites W2015637674 @default.
- W2897414813 cites W2021956736 @default.
- W2897414813 cites W2024081693 @default.
- W2897414813 cites W2028704213 @default.
- W2897414813 cites W2036121739 @default.
- W2897414813 cites W2052151970 @default.
- W2897414813 cites W2056718431 @default.
- W2897414813 cites W2063027921 @default.
- W2897414813 cites W2065529157 @default.
- W2897414813 cites W2068262275 @default.
- W2897414813 cites W2080907069 @default.
- W2897414813 cites W2083352943 @default.
- W2897414813 cites W2090459210 @default.
- W2897414813 cites W2096245028 @default.
- W2897414813 cites W2096882371 @default.
- W2897414813 cites W2097088124 @default.
- W2897414813 cites W2098564368 @default.
- W2897414813 cites W2100569210 @default.
- W2897414813 cites W2106418369 @default.
- W2897414813 cites W2116219980 @default.
- W2897414813 cites W2117644792 @default.
- W2897414813 cites W2119131940 @default.
- W2897414813 cites W2124199755 @default.
- W2897414813 cites W2125489913 @default.
- W2897414813 cites W2126377049 @default.
- W2897414813 cites W2139937287 @default.
- W2897414813 cites W2148228095 @default.
- W2897414813 cites W2149078886 @default.
- W2897414813 cites W2156048499 @default.
- W2897414813 cites W2156709532 @default.
- W2897414813 cites W2158622701 @default.
- W2897414813 cites W2167562984 @default.
- W2897414813 cites W2176532917 @default.
- W2897414813 cites W2216753448 @default.
- W2897414813 cites W2296455390 @default.
- W2897414813 cites W2297215020 @default.
- W2897414813 cites W2301117188 @default.
- W2897414813 cites W2410852485 @default.
- W2897414813 cites W2460998372 @default.
- W2897414813 cites W2479266419 @default.
- W2897414813 cites W2508402256 @default.
- W2897414813 cites W2524618357 @default.
- W2897414813 cites W2575003957 @default.
- W2897414813 cites W2575788199 @default.
- W2897414813 cites W2593844102 @default.
- W2897414813 cites W2600163159 @default.
- W2897414813 cites W2612049161 @default.
- W2897414813 cites W2768653164 @default.
- W2897414813 cites W2782426885 @default.
- W2897414813 cites W2800817650 @default.
- W2897414813 cites W2803145019 @default.
- W2897414813 cites W2803262790 @default.
- W2897414813 cites W2953228579 @default.
- W2897414813 cites W3098221464 @default.
- W2897414813 cites W3099273144 @default.
- W2897414813 cites W3099471130 @default.
- W2897414813 cites W3099684615 @default.
- W2897414813 cites W3100007886 @default.
- W2897414813 cites W3100110286 @default.
- W2897414813 cites W3100195645 @default.
- W2897414813 cites W3100240161 @default.
- W2897414813 cites W3101144084 @default.
- W2897414813 cites W3101374472 @default.
- W2897414813 cites W3101771129 @default.
- W2897414813 cites W3103112373 @default.