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Table 7

Nine late type stars,which ULySS could not successfully fit.

Name Sp. Type T eff log (g) [Fe/H] Ref.
(K) cm   s-2 (dex)

HD 078712 M6IIIase 3210 0.00 –0.01 A
3101 0.23 –1.00 0
3210 0.00 –0.11 1
3210 0.00 0.09 1
HD 084748 M8IIIe 3070 0.78 –1.00 0&A
HD 114961 M7III 3014 0.00 –0.81 2&A
3080 0.36 –1.00 0
HD 126327 M7.5 3000 0.00 –0.58 2&A
3088 0.30 –1.00 0
HD 148783 M6III 3250 0.20 –0.04 A
3146 0.45 –1.00 0
3250 0.20 –0.01 3
3250 0.20 –0.06 4
HD 177940 M7IIIevar 3092 0.59 –1.00 0&A
HD 187796 S... 3148 0.49 –1.00 0&A
HD 196610 M6III 3100 0.39 –1.00 0&A
HD 197812 M5Iab: 3389 0.32 –1.00 A
3119 0.32 –1.00 0
3389 5

Notes. First column is the star name. Second column is the stellar spectral type. Third to fifth column are the three atmospheric parameters. Sixth lists the source of the measurements. For HD 78712 we adopt the averaged parameters from Smith & Lambert (1986)’s two solutions, for HD 114961 and 126327 we adopt values from Jones (1999), for HD 148783 we adopt the averaged values of Ramírez et al. (2000) and Carr et al. (2000), for HD 197812 we use the Teff value from Dyck et al. (1998), and adopt log g and [Fe/H] value of ULySS determination. For the remaining four stars, as no other reference could be found, we adopt our determinations in the final table.

References. (A) Adopted solution; (0) ULySS fit to the CFLIB spectrum; (1) Smith & Lambert (1986); (2) Jones (1999); (3) Ramírez et al. (2000); (4) Carr et al. (2000); (5) Dyck et al. (1998).

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