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.

field RASS name Sp. type EW(Li I ) $\log N$ (Li) $v~\sin i$

[mÅ] [km s^-1]

A010 RX J0331.1+0713 K4Ve 407 3.08 42

A057 RX J0344.4-0123 G9V-IV 277 3.23 20

A058 RX J0344.8+0359 K1Ve 310 3.17 31

A069 RX J0348.5+0831 G4V: 259 3.59 >100

A094 RX J0355.2+0329 K3V 424 3.39 >100

A100 RX J0358.1-0121 K4V 362 2.84 15

A104 RX J0400.1+0818 G5V-IV 259 3.49 12

A161 RX J0417.8+0011 M0Ve 304 1.48 44

B002 $^{\ast}$ RX J0638.9+6409 K3III 315 2.17 6

B026 RX J0708.7+6135 M4e 272 0.53 *

B206 RX J0828.1+6432 K8Ve 607 3.06 16

F140 $^{\ast}$ RX J2241.9+1431 K0III 307 3.36 <5

**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.
field	RASS name	Sp. type	EW(Li I )	$\log N$ (Li)	$v~\sin i$
			[mÅ]		[km s^-1]
A010	RX J0331.1+0713	K4Ve	407	3.08	42
A057	RX J0344.4-0123	G9V-IV	277	3.23	20
A058	RX J0344.8+0359	K1Ve	310	3.17	31
A069	RX J0348.5+0831	G4V:	259	3.59	>100
A094	RX J0355.2+0329	K3V	424	3.39	>100
A100	RX J0358.1-0121	K4V	362	2.84	15
A104	RX J0400.1+0818	G5V-IV	259	3.49	12
A161	RX J0417.8+0011	M0Ve	304	1.48	44
B002 $^{\ast}$	RX J0638.9+6409	K3III	315	2.17	6
B026	RX J0708.7+6135	M4e	272	0.53	*
B206	RX J0828.1+6432	K8Ve	607	3.06	16
F140 $^{\ast}$	RX J2241.9+1431	K0III	307	3.36	<5

Source LaTeX | All tables | In the text

	1 Introduction
	2 The sample
	3 Spectroscopic observations
	4 Observational results
	5 Data analysis and discussion
	6 Conclusions
	Appendix A: Parameters of the sample and results
	References
	Online Material