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Table 1

Parameters of the observed solar analogues in M 67.

Object (L/L) log N(Li)NLTE log N(Li)moog*
(K)

285 5836  ±  67  <0.6 0.6
637 5806  ±  65 1.4 1.5
1101 5756  ±  60  <0.6  <0.6
1194 5766  ±  64  <0.6  <1.3
1303 5716  ±  64  <0.6 1.2
1304 5704  ±  64  <0.5  <0.8
1315 5874  ±  58 1.4 1.8
1392 5716  ±  63  <0.6  <0.6
1787 5768  ±  70 1.0 1.6
2018 5693  ±  74  <0.5  <1.3

Notes. Cols. 1–4 from Pasquini et al. (2008).

*

Our determinations of the Li abundances using the MOOG program.

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