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Fig. 5

image

Heliocentric radial velocity density distributions in the field centred at l = 0° and b = −6° for stars in the near and far sides of the bar. Only disk stars with | x | ≤ 2.5 kpc and | y | ≤ 3 kpc were selected. The size of the field is Δl = Δb = 1°. Curves in blue and in red correspond to stars born at rini< 2.5 kpc and at 2.5 kpc rini< 4.5 kpc, respectively, at the bright (dotted line) and faint (solid line) sides of the bar.

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