A Role for Turbulence in Circumgalactic Precipitation
A Role for Turbulence in Circumgalactic Precipitation
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DOI:
10.3847/1538-4357/aae8e2
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发表时间:
2018-03
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影响因子:
--
通讯作者:
G. Voit
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文献类型:
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作者:
G. Voit
The cooling time, tcool, of the hot ambient medium pervading a massive galaxy does not drop much below 10 times the freefall time tff at any radius. Theoretical models have accounted for this finding by hypothesizing that cold clouds start to condense out of the ambient medium when tcool/tff ≲ 10 and fuel a strong black hole feedback response, but they have not yet provided a simple explanation for the critical tcool/tff ratio. This paper explores a heuristic model for condensation linking the critical ratio to turbulent driving of gravity wave oscillations. In the linear regime, internal gravity waves are thermally unstable in a thermally balanced medium. Buoyancy oscillations in a balanced medium with tcool/tff ≫ 1 therefore grow until they saturate without condensing at an amplitude depending on tcool/tff. However, in a medium with 10 ≲ tcool/tff ≲ 20, turbulence with a velocity dispersion roughly half the galaxy’s stellar velocity dispersion can drive those oscillations into condensation. Intriguingly, this is indeed the gas-phase velocity dispersion observed among multiphase galaxy cluster cores. It is therefore possible that both the critical tcool/tff ratio for condensation of ambient gas and the level of turbulence in that gas are determined by coupling between condensation, feedback, and turbulence. Such a system can converge to a well-regulated equilibrium state, if the fraction of feedback energy going into turbulence is subdominant.