Azimuthal dependence of the density distribution in outer galactic discs accreting intergalactic flows
Aims: The amplitude and scaleheight of the Galactic gas disc density are not axisymmetric against expectations in a self-gravity axisymmetric disc. However, this lopsidedness can be explained in terms of intergalactic accretion flows, which produce non-axisymmetric pressure on the disc. This mechanism could be also responsible for the formation of
López-Corredoira, M. et al.
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2009