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Influence of inelastic collisions with hydrogen atoms on the non-LTE modelling of Ca i and Ca ii lines in late-type stars | Astronomy & Astrophysics (A&A)
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Table 3

Atmospheric parameters and obtained calcium NLTE and LTE abundances of the UMP stars.

HE Teff log g [Fe/H] Vmic Ref. NLTE, log εCa LTE, log εCa


[K] [km s-1] Ca i 4226 Å Ca ii Ca i 4226 Å Ca ii

0107-5240 5100 2.2 5.3 2.2 CGK04 1.28 1.38 0.94 1.41
0557-4840 4900 2.2 4.75 1.8 NCK07 1.94 2.20 (5, 0.05) 1.78 2.55 (5, 0.37)
1327-2326 6180 3.7 5.45 1.7 AFC06 1.16 1.18 (2, 0.02) 0.91 1.33 (2, 0.06)

Notes. Ref.: AFC06 = Aoki et al. (2006), CGK04 = Christlieb et al. (2004), NCK07 = Norris et al. (2007). Numbers in parenthesis indicate the number of lines measured and σ.

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