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Table 3:

Summary of the bulge minor axis fields (Paper I) characteristics. $z_{\rm GC}$ is the height of the field along the bulge minor axis, assuming a distance Sun - Galactic Centre of 8 kpc.

Field 		l b $z_{\rm GC}$ N $\langle V_{\rm r} \rangle$ $\sigma _{\rm r}$ Skew Kurtosis
  ($^\circ$) ($^\circ$) (pc)   (km s-1) (km s-1)    
$b=-4\hbox {$^\circ $ }$ 1.1 -4.0 606 194    5 $\pm$ 7 104 $\pm$ 5 $-0.07 \pm 0.1$ $-0.54 \pm 0.2$
$b=-6\hbox {$^\circ $ }$ 0.2 -6.0 844 201 $-10 \pm 6$  83 $\pm$ 4  0.01 $\pm$ 0.1 $-0.19 \pm 0.2$
$b=-12\hbox{$^\circ$ }$ 0.0 -12.0 1700 99 $-14 \pm 8$  80 $\pm$ 8  0.38 $\pm$ 0.4  1.71 $\pm$ 0.7

Notes. N is the number of stars. $\langle V_{\rm r} \rangle$is the mean heliocentric velocity.


Source LaTeX | All tables | In the text

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