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- W3103138619 endingPage "L30" @default.
- W3103138619 startingPage "L30" @default.
- W3103138619 abstract "Galaxy growth depends critically on the interplay between radiative cooling of cosmic gas and the resulting energetic feedback that cooling triggers. This interplay has proven exceedingly difficult to model, even with large supercomputer simulations, because of its complexity. Nevertheless, real galaxies are observed to obey simple scaling relations among their primary observable characteristics. Here we show that a generic emergent property of the interplay between cooling and feedback can explain the observed scaling relationships between a galaxy's stellar mass, its total mass, and its chemical enrichment level, as well as the relationship between the average orbital velocity of its stars and the mass of its central black hole. These relationships naturally result from any feedback mechanism that strongly heats a galaxy's circumgalactic gas in response to precipitation of colder clouds out of that gas, because feedback then suspends the gas in a marginally precipitating state." @default.
- W3103138619 created "2020-11-23" @default.
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- W3103138619 date "2015-07-23" @default.
- W3103138619 modified "2023-10-13" @default.
- W3103138619 title "PRECIPITATION-REGULATED STAR FORMATION IN GALAXIES" @default.
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- W3103138619 doi "https://doi.org/10.1088/2041-8205/808/1/l30" @default.
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