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3D Hydrodynamical Simulations of a Galactic Fountain
Published online by Cambridge University Press: 12 April 2016
Abstract
Galactic fountains are thought to be responsible for the formation of the observed intermediate and high velocity clouds in the Galactic halo. Threedimensional simulations have been carried out to determine the evolution of the disk gas as it enters the fountain, cools and returns to the Galactic disk. The descending cold gas, headed by a shock, sweeps up the ascending flow, triggering the formation of an unstable layer where Rayleigh-Taylor instabilities grow, which may provoke the formation of the observed clouds.
- Type
- Part VIII High-Velocity Clouds, Galactic Halo Models, Observations of the LMC
- Information
- International Astronomical Union Colloquium , Volume 166: The Local Bubble and Beyond , 1997 , pp. 495 - 498
- Copyright
- Copyright © Springer-Verlag 1998