All Tables

Table 1: Journal of observations.
Table 2: Revised and original statistics of the distribution of spectral type among the RASS sources with stellar counterparts of spectral types F to M.
Table 3: Spectroscopic MK standard stars. The spectral types are listed in column "sp. type''. References for the spectral types are given in column "ref.'': 1 = Yamashita et al. (1976), 2 = Gray et al. (2001), 3 = Keenan & Barnbaum (1999), 4 = Garcia (1989), 5 = Keenan & McNeil (1989), 6 = Prugniel & Soubiran (2001).
Table 4: Median $v\sin i$ (in km s^-1) for the different age groups. Giants were not included in group Hya+.
Table 5: Spectral types, lithium equivalent widths, EW(Li), logarithmic abundances, $\log N$ (Li), and projected rotational velocities for the subsample of stars with lithium abundance above the Pleiades upper envelope. ("PMS'' sample). Evolved lithium-rich stars not belonging to the PMS sample are marked by the " ${\ast }$ '' symbol.
Table 6: Spectral types, lithium equivalent widths, EW(Li), logarithmic abundances, $\log N$ (Li), and projected rotational velocities for the subsample of stars with lithium abundance between the Pleiades lower and upper envelope ("Pl_ZAMS'' sample). Lithium-rich evolved stars not belonging to the Pl_ZAMS sample are marked by " ${\ast }$ ''.
Table 7: Statistics of the age distribution of the sample of G-K stars. "PMS'' denotes stars younger than 100 Myr, "Pl_ZAMS'' stars as old as the Pleiades, "UMa'' stars with an age of $\sim 300$ Myr, and "Hya+'' older than the Hyades. The latter age group also contains 17 evolved stars (LC IV-III, III, and II). The total number of G-K stars is 141.
Table 8: Statistics of the spatial distribution of the various age groups in the sample. For each age group the total number of stars and the number per square degree is given. The numbers are for a RASS count-rate limit of 0.03 cts s^-1except for area V which has a count-rate limit of 0.01 cts s^-1.
Table 9: Mean proper motions and dispersions in area I for stars of age groups PMS, Pl_ZAMS, UMa, and M stars without lithium detection (in mas yr^-1).
Table 10: Mean proper motions (in mas s^-1), and mean tangential velocities (in km s^-1) in galactic coordinates, both with dispersions, reduced to the LSR. The values are listed for stars of the age groups PMS, Pl_ZAMS, UMa and Hya+ (split into dwarfs and giants), and M stars without lithium detection.
Table 11: Mean (M-L) space velocity components, $\langle U\rangle, \langle V\rangle, \langle W\rangle$ , and velocity dispersions, $\sigma _U$ , $\sigma _V$ , $\sigma _W$ , of the different age groups in km s^-1.
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.
Table A.2: Basic optical and X-ray parameters of the sample of G-, K-, and M-type stars.
Table A.3: Kinematical parameters.
Table A.4: Lithium abundances and rotational velocities.