**Table 2:** The fit results of the z-probability distribution from Fig. 7. Scale heights and number densities are given for each fitted component. For a two-component fit no "thick disk'' values were determined.
fit constants	2 comp.	3 comp.
$h_{\rm thin}$ [kpc]	0.1	0.12
$N_{\rm thin}(0)^a$	5.5 $\times$ 10⁶	4.8 $\times$ 10⁶
$h_{\rm thick}$ [kpc]	-	0.58
$N_{\rm thick}(0)^a$	-	51 000
$h_{\rm halo}~[{\rm kpc}]^b$	5	4.2
$N_{\rm halo}(0)^{a,b}$	1100	900

^a Values of N(0) come from the numerics of the orbit statistics
and cannot be used as number of stars per unit volume.
^b Halo values are based on three stars only (see Sect. 4.3).

Source LaTeX | All tables | In the text

	1 Introduction
	2 Establishing the RHB data sample
	3 Error limits and selection effects
	4 The spatial distribution of RHB stars
	5 Effects of galactic mass models
	6 Comparing the distribution of RHB stars with other types
	References