All Tables

Table 1: Stellar parameters of the high mass CSPN from PHM, heliocentric radial velocities (from Durand et al. 1998) and proper motion measurements. The last column gives the source of the proper motion values.
Table 2: Adopted velocity dispersions $\sigma _U$ , $\sigma _V$ , $\sigma _W$ and asymmetric drift $v_{{\rm ad}}$ for the young thin disk (YTD), the old thin disk (OTD) and for the thick disk (from Robin et al. 2003).
Table 3: Nebular abundances for the very high mass CSPN of the PHM sample.