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- W2082565287 abstract "Accretion of fresh gas at a rate of ∼ 1M☉yr−1 is necessary in star-forming disc galaxies, such as the Milky Way, in order to sustain their star-formation rates. In this work we present the results of a new hydrodynamic simulation supporting the scenario in which the gas required for star formation is drawn from the hot corona that surrounds the star-forming disc. In particular, the cooling of this hot gas and its accretion on to the disc are caused by the passage of cold galactic fountain clouds through the corona." @default.
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- W2082565287 date "2012-01-01" @default.
- W2082565287 modified "2023-09-26" @default.
- W2082565287 title "Fountain-driven gas accretion by the Milky Way" @default.
- W2082565287 doi "https://doi.org/10.1051/epjconf/20121908008" @default.
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