Table 5: Final temperatures as derived from different reddening corrections. The whole table is available on-line.

HIP		 Effective temperature scales (K)
  2 1 3 4 S98 H97
Sample #1: the clean sample

911		 5972 5918 5972 5972 6076 6065
3026 6040 6026 6040 6040 6221 6214
3446 5901 5901 5894 5901 5991 5995
3564 5683 5683 5683 5683 5974 5679
8572 6287 6287 6287 6287 6265 6287
... ... ... ... ... ... ...

Sample #2: the $\beta $ sample

484		 5064 5064 5064 5064 5064 ...
3554 5008 5008 5008 5008 5040 5022
4343 5064 5064 5064 5064 5069 5064
8314 6430 6430 6430 6430 ... 6444
13 749 4965 4965 4965 4965 4996 4965
... ... ... ... ... ... ...

Sample #3: the ubvy sample

12 807		 5932 5932 5932 5932 6872: 5959
83 320 5984 5984 5984 5984 6251 5861
87 062 5909 5909 5909 5909 ... 5905
91 129 6217 6217 6217 6217 7081: 6237
103 337 4885 4885 4885 4885 4876 4876
... ... ... ... ... ... ...


Source LaTeX | All tables | In the text

Article Contents
1 The lithium paradigm
2 The "Lithium plateau debate''?
3 Sample selection: a critical analysis of the literature
4 Stellar parameters: I. Gravity, metallicity, and microturbulence
5 Stellar parameters. II. The temperature scale and its weaknesses
6 Our final choice: temperature and data-sample(s)
7 The lithium abundance
8 Preliminary results on the mean lithium abundance and the dispersion
9 Evolutionary status of the stars
10 The lithium abundance along the plateau for the dwarf stars
11 The lithium abundance in evolved stars
12 Duplicity and variability
13 Stars with extreme Li abundances
14 Implications for stellar structure and evolution
15 Summary and conclusions
References
Online Material
List of tables
List of figures