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Fig. 7

image

Dependency of observable Galactic latitude b (black) and projected vertical velocity (blue) on heliocentric distance x for a plane-parallel slab of fountain objects at vertical scale height z = +2 kpc with a downward motion of vz = −100 km s-1. The 1D heliocentric distance x is measured within the plane of the disk. The vertical and horizontal lines indicate the limits of our search for MIVCs of 20 km s-1 ≤ | vLSR | ≤ 100 km s-1 and | b | > 20°. The coloured areas show the observable parameter spaces.

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