Table A.1: Mean tangential velocities and dispersions (in km s^-1) in galactic coordinates for stars of age groups PMS, Pl_ZAMS, UMa, Hya+ (split into dwarfs and giants), and M stars without lithium detection for the individual study areas. The first two lines give the average solar velocity for each study area. The mean distance $\langle d \rangle$ and its scatter are given in pc. The number of stars used for the calculation of the mean values are given in parentheses.

area I II III IV V VI

$\langle v_{l,\odot} \rangle$ -4 -9 +8 -5 -11 -8

$\langle v_{b,\odot} \rangle$ -0 +10 +11 +10 +4 +11

PMS:

$\langle v_l \rangle$ $+9 \pm 9 (8)$ $+7 \pm 2$ (2) - - - -

$\langle v_b \rangle$ $+5 \pm 11$ (8) $-3 \pm 1$ (2) - - - -

$\langle d \rangle$ $121 \pm 53$ (8) $51 \pm 20$ (2) - - - -

Pl_ZAMS:

$\langle v_l \rangle$ $+11 \pm 13$ (13) $+13 \pm 4$ (8) $-6 \pm 8$ (6) - $+52 \pm 26$ (3) $+2 \pm 4$ (6)

$\langle v_b \rangle$ $-1 \pm 15$ (13) $-5 \pm 7$ (8) $-19 \pm 11$ (6) - $+7 \pm 19$ (3) $-6 \pm 12$ (6)

$\langle d \rangle$ $118 \pm 56$ (14) $117 \pm 50$ (9) $91 \pm 39$ (7) - $226 \pm 191$ (3) $101 \pm 77$ (6)

UMa:

$\langle v_l \rangle$ $+4 \pm 13$ (2) - - $-24 \pm 42$ (6) $-10 \pm 18$ (6)

$\langle v_b \rangle$ $-10 \pm 12$ (2) - - $-10 \pm 21$ (6) $-7 \pm 8$ (6)

$\langle d \rangle$ $323 \pm 191$ (3) - - $332 \pm 252$ (6) $240 \pm 184$ (6)

Hya+:

dwarfs:

$\langle v_l \rangle$ $+3 \pm 12$ (8) $+4 \pm 17$ (6) $-6 \pm 39$ (9) $+11 \pm 23$ (4) $+12 \pm 15$ (3) $-11 \pm 45$ (4)

$\langle v_b \rangle$ $-5 \pm 15$ (8) $-9 \pm 9$ (6) $-15\pm 16$ (9) $-2 \pm 26$ (4) $-3 \pm 8$ (3) $-24 \pm 36$ (4)

$\langle d \rangle$ $82 \pm 46$ (8) $132 \pm 165$ (6) $90 \pm 56$ (9) $204 \pm 102$ (4) $56 \pm 45$ (3) $201 \pm 245$ (4)

giants:

$\langle v_l \rangle$ $-2 \pm 12$ (2) $+11 \pm 93$ (10) - - $+6 \pm 21$ (2) -

$\langle v_b \rangle$ $+7 \pm 7$ (2) $-8 \pm 42$ (10) - - $+15 \pm 19$ (2) -

$\langle d \rangle$ $124 \pm 26$ (2) $601 \pm 810$ (10) - - $175 \pm 101$ (2) -

M stars:

$\langle v_l \rangle$ $+12 \pm 10$ (12) $0 \pm 21$ (5) $-8 \pm 16$ (10) $-3 \pm 27$ (6) $+6 \pm 27$ (8) $+10 \pm 18$ (7)

$\langle v_b \rangle$ $+0 \pm 9$ (12) $+5 \pm 16$ (5) $-15 \pm 15$ (10) $-44 \pm 35$ (6) $-10 \pm 27$ (8) $-19 \pm 11$ (7)

$\langle d \rangle$ $43 \pm 30$ (14) $60 \pm 24$ (6) $56 \pm 32$ (11) $53 \pm 27$ (6) $59 \pm 23$ (8) $43 \pm 15$ (7)

**Table A.1:** Mean tangential velocities and dispersions (in km s^-1) in galactic coordinates for stars of age groups PMS, Pl_ZAMS, UMa, Hya+ (split into dwarfs and giants), and M stars without lithium detection for the individual study areas. The first two lines give the average solar velocity for each study area. The mean distance $\langle d \rangle$ and its scatter are given in pc. The number of stars used for the calculation of the mean values are given in parentheses.
area	I	II	III	IV	V	VI
$\langle v_{l,\odot} \rangle$	-4	-9	+8	-5	-11	-8
$\langle v_{b,\odot} \rangle$	-0	+10	+11	+10	+4	+11
PMS:
$\langle v_l \rangle$	$+9 \pm 9 (8)$	$+7 \pm 2$ (2)	-	-	-	-
$\langle v_b \rangle$	$+5 \pm 11$ (8)	$-3 \pm 1$ (2)	-	-	-	-
$\langle d \rangle$	$121 \pm 53$ (8)	$51 \pm 20$ (2)	-	-	-	-
Pl_ZAMS:
$\langle v_l \rangle$	$+11 \pm 13$ (13)	$+13 \pm 4$ (8)	$-6 \pm 8$ (6)	-	$+52 \pm 26$ (3)	$+2 \pm 4$ (6)
$\langle v_b \rangle$	$-1 \pm 15$ (13)	$-5 \pm 7$ (8)	$-19 \pm 11$ (6)	-	$+7 \pm 19$ (3)	$-6 \pm 12$ (6)
$\langle d \rangle$	$118 \pm 56$ (14)	$117 \pm 50$ (9)	$91 \pm 39$ (7)	-	$226 \pm 191$ (3)	$101 \pm 77$ (6)
UMa:
$\langle v_l \rangle$	$+4 \pm 13$ (2)	-	-		$-24 \pm 42$ (6)	$-10 \pm 18$ (6)
$\langle v_b \rangle$	$-10 \pm 12$ (2)	-	-		$-10 \pm 21$ (6)	$-7 \pm 8$ (6)
$\langle d \rangle$	$323 \pm 191$ (3)	-	-		$332 \pm 252$ (6)	$240 \pm 184$ (6)
Hya+:
dwarfs:
$\langle v_l \rangle$	$+3 \pm 12$ (8)	$+4 \pm 17$ (6)	$-6 \pm 39$ (9)	$+11 \pm 23$ (4)	$+12 \pm 15$ (3)	$-11 \pm 45$ (4)
$\langle v_b \rangle$	$-5 \pm 15$ (8)	$-9 \pm 9$ (6)	$-15\pm 16$ (9)	$-2 \pm 26$ (4)	$-3 \pm 8$ (3)	$-24 \pm 36$ (4)
$\langle d \rangle$	$82 \pm 46$ (8)	$132 \pm 165$ (6)	$90 \pm 56$ (9)	$204 \pm 102$ (4)	$56 \pm 45$ (3)	$201 \pm 245$ (4)
giants:
$\langle v_l \rangle$	$-2 \pm 12$ (2)	$+11 \pm 93$ (10)	-	-	$+6 \pm 21$ (2)	-
$\langle v_b \rangle$	$+7 \pm 7$ (2)	$-8 \pm 42$ (10)	-	-	$+15 \pm 19$ (2)	-
$\langle d \rangle$	$124 \pm 26$ (2)	$601 \pm 810$ (10)	-	-	$175 \pm 101$ (2)	-
M stars:
$\langle v_l \rangle$	$+12 \pm 10$ (12)	$0 \pm 21$ (5)	$-8 \pm 16$ (10)	$-3 \pm 27$ (6)	$+6 \pm 27$ (8)	$+10 \pm 18$ (7)
$\langle v_b \rangle$	$+0 \pm 9$ (12)	$+5 \pm 16$ (5)	$-15 \pm 15$ (10)	$-44 \pm 35$ (6)	$-10 \pm 27$ (8)	$-19 \pm 11$ (7)
$\langle d \rangle$	$43 \pm 30$ (14)	$60 \pm 24$ (6)	$56 \pm 32$ (11)	$53 \pm 27$ (6)	$59 \pm 23$ (8)	$43 \pm 15$ (7)

Source LaTeX | All tables | In the text

	1 Introduction
	2 The sample
	3 Spectroscopic observations
	4 Observational results
	5 Data analysis and discussion
	6 Conclusions
	Appendix A: Parameters of the sample and results
	References
	Online Material