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 " ${\ast }$ ''.

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

[mÅ] [km s^-1]

A001 RX J0328.2+0409 K0 275 3.12 96

A036 RX J0338.7+0136 K4Ve 80 1.08 17

A039 RX J0338.8+0216 K4 58 0.90 16

A042 RX J0339.9+0314 K2 104 1.64 63

A056 RX J0343.9+0327 K1V-IV 126 1.97 12

A063 RX J0347.1-0052 K3V 84 1.31 21

A071 RX J0348.9+0110 K3V:e 258 2.36 83

A090 RX J0354.3+0535 G0V 131 3.03 31

A095 RX J0355.3-0143 G5V 213 3.16 19

A096 RX J0356.8-0034 K3V 122 1.55 22

A101 RX J0358.9-0017 K3V 294 2.62 27

A120 RX J0404.4+0518 G7V 239 3.15 27

A126 RX J0405.6+0341 G0V-IV 63 2.54 < 5

A154 RX J0416.2+0709 G0V 58 2.50 11

B008 RX J0648.5+6639 G5 121 2.58 9

B018 RX J0704.0+6214 K5Ve 36 0.50 12

B034 $^{\ast}$ RX J0714.8+6208 G1IV-III 127 2.93 12

B039 RX J0717.4+6603 K2V 213 2.27 21

B068 RX J0732.3+6441 K5e 130 1.21 *

B086 $^{\ast}$ RX J0742.8+6109 K0III 147 1.65 11

B124 $^{\ast}$ RX J0755.8+6509 G5III 153 2.19 6

B160 RX J0809.2+6639 G2V 128 2.86 12

B174 RX J0814.5+6256 G1V 136 2.99 11

B183 RX J0818.3+5923 K0V 134 2.21 7

B185 RX J0819.1+6842 K7Ve 26 0.02 13

B199 RX J0824.5+6453 K4V 50 0.83 26

C047 RX J1027.0+0048 G0V 73 2.63 11

C058 RX J1028.6-0127 K5e 30 0.41 12

C143 RX J1051.3-0734 K2V 75 1.44 18

C165 RX J1057.1-0101 K4V 34 0.65 7

C176 RX J1059.7-0522 K1V 148 2.09 9

C197 RX J1104.6-0413 G5V 130 2.64 10

C200 RX J1105.3-0735 K5e 160 1.38 32

D064 RX J1210.6+3732 K0 115 2.10 19

E022 RX J1628.4+7401 G1V 172 3.21 18

E067 RX J1653.5+7344 G1IV 98 2.43 8

E179 RX J1728.1+7239 K4IVe 66 0.53 18

F015 RX J2156.4+0516 K2 185 2.11 12

F046 RX J2212.2+1329 G8:V: 106 2.23 5

F060 RX J2217.4+0606 K1e 108 1.86 8

F087 RX J2226.3+0351 G5:V: 80 2.31 31

F101 RX J2232.9+1040 K2V: 285 2.76 97

F142 RX J2242.0+0946 K8V 54 0.26 24

**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 " ${\ast }$ ''.
field	RASS name	Sp. type	EW(Li I )	$\log N$ (Li)	$v~\sin i$
			[mÅ]		[km s^-1]
A001	RX J0328.2+0409	K0	275	3.12	96
A036	RX J0338.7+0136	K4Ve	80	1.08	17
A039	RX J0338.8+0216	K4	58	0.90	16
A042	RX J0339.9+0314	K2	104	1.64	63
A056	RX J0343.9+0327	K1V-IV	126	1.97	12
A063	RX J0347.1-0052	K3V	84	1.31	21
A071	RX J0348.9+0110	K3V:e	258	2.36	83
A090	RX J0354.3+0535	G0V	131	3.03	31
A095	RX J0355.3-0143	G5V	213	3.16	19
A096	RX J0356.8-0034	K3V	122	1.55	22
A101	RX J0358.9-0017	K3V	294	2.62	27
A120	RX J0404.4+0518	G7V	239	3.15	27
A126	RX J0405.6+0341	G0V-IV	63	2.54	< 5
A154	RX J0416.2+0709	G0V	58	2.50	11
B008	RX J0648.5+6639	G5	121	2.58	9
B018	RX J0704.0+6214	K5Ve	36	0.50	12
B034 $^{\ast}$	RX J0714.8+6208	G1IV-III	127	2.93	12
B039	RX J0717.4+6603	K2V	213	2.27	21
B068	RX J0732.3+6441	K5e	130	1.21	*
B086 $^{\ast}$	RX J0742.8+6109	K0III	147	1.65	11
B124 $^{\ast}$	RX J0755.8+6509	G5III	153	2.19	6
B160	RX J0809.2+6639	G2V	128	2.86	12
B174	RX J0814.5+6256	G1V	136	2.99	11
B183	RX J0818.3+5923	K0V	134	2.21	7
B185	RX J0819.1+6842	K7Ve	26	0.02	13
B199	RX J0824.5+6453	K4V	50	0.83	26
C047	RX J1027.0+0048	G0V	73	2.63	11
C058	RX J1028.6-0127	K5e	30	0.41	12
C143	RX J1051.3-0734	K2V	75	1.44	18
C165	RX J1057.1-0101	K4V	34	0.65	7
C176	RX J1059.7-0522	K1V	148	2.09	9
C197	RX J1104.6-0413	G5V	130	2.64	10
C200	RX J1105.3-0735	K5e	160	1.38	32
D064	RX J1210.6+3732	K0	115	2.10	19
E022	RX J1628.4+7401	G1V	172	3.21	18
E067	RX J1653.5+7344	G1IV	98	2.43	8
E179	RX J1728.1+7239	K4IVe	66	0.53	18
F015	RX J2156.4+0516	K2	185	2.11	12
F046	RX J2212.2+1329	G8:V:	106	2.23	5
F060	RX J2217.4+0606	K1e	108	1.86	8
F087	RX J2226.3+0351	G5:V:	80	2.31	31
F101	RX J2232.9+1040	K2V:	285	2.76	97
F142	RX J2242.0+0946	K8V	54	0.26	24

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