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Redistributing hot gas around galaxies: do cool clouds signal a solution to the overcooling problem?

Monthly Notices of the Royal Astronomical Society, no. 1 (2009): 191-202

Cited: 71|Views28

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hydrodynamicsmethods: N-body simulationsmethods: numericalgalaxies: formation

Abstract

We present a pair of high-resolution smoothed particle hydrodynamics simulations that explore the evolution and cooling behaviour of hot gas around Milky Way size galaxies. The simulations contain the same total baryonic mass and are identical other than their initial gas density distributions. The first is initialized with a low-entropy ...More

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