Table 3: Characteristics of the stars located in the region $L_{xy}^{\rm min}<L_{xy}<L_{xy}^{\rm max}$ and $L_z^{\rm min}<L_z<L_z^{\rm max}$ defined by the Helmi et al. (1999) structure (within the box shown in the left panel of Fig. 6.)
Name $\rm {[Fe/H]}$ E/105 Lz Lxy e Membership
  (dex) ( $\rm {km^2~s^{-2}}$) ( $\rm {kpc~km~s^{-1}}$) ( $\rm {kpc~km~s^{-1}}$)    
BPS CS 22948-0093 -3.72 -0.57 687 1805 0.92  
HD 214161 -2.16 -0.73 952 2173 0.81 RHLS
V* RZ Cep -1.77 -0.77 710 1943 0.85 RHLS
BPS CS 30339-0037 -2.13 -0.87 586 1909 0.81 RHLS
BPS CS 22189-0007 -2.12 -0.97 683 1624 0.77  
BPS CS 29513-0031 -2.79 -1.00 1171 2189 0.47 CB
BD+10 2495 -1.83 -1.02 1318 2140 0.47 HWdZZ, CB
HD 119516 -2.49 -1.04 1212 2055 0.50 HWdZZ, CB
V* TT Cnc -1.57 -1.06 562 2483 0.42 HWdZZ
CD-36 1052 -2.19 -1.06 1078 2132 0.45 HWdZZ, CB
HD 237846 -2.63 -1.09 774 1443 0.71 HWdZZ
BPS CS 29504-0044 -2.04 -1.10 958 2091 0.42 CB
V* AR Ser -1.78 -1.12 322 1934 0.46 HWdZZ
V* TT Lyn -1.56 -1.11 748 2124 0.45 HWdZZ, CB
HD 128279 -2.20 -1.18 1194 1844 0.23 HWdZZ, CB
BPS CS 22876-0040 -2.20 -1.19 922 1561 0.42 CB


Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Halo samples from the Beers et al. (2000) catalog
3 Kinematic analysis
4 Comparison to the theory: simulations
5 Adiabatic invariants
6 Conclusions
References
List of tables
List of figures