All Tables

Table 1: Rate coefficients $\langle \sigma v \rangle$ , in units of cm³ s^-1, for the processes H(1s) + Li(nl) $\rightarrow$ H(1s) + Li( $n^\prime l^\prime$ ), or where indicated H(1s) + Li(nl) $\rightarrow$ H^- + Li⁺(1s²) and H^- + Li⁺(1s²) $\rightarrow$ H(1s) + Li( $n^\prime l^\prime$ ), for selected temperatures in the range T=2000-8000 K. Asterisks indicate transitions where the calculated cross sections are considered unreliable.
Table 2: Predicted flux equivalent widths (in pm = 10 mÅ) for the 670.8 nm line in the Sun, HD 140283 and HD 84937 based on 1D and 3D models, in both LTE and non-LTE. Results are shown for various model atoms as described in the text. Note that the 3D results shown are based on only one snapshot and hence are not appropriate for a direct comparison with the 1D cases.