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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