All Tables

Table 1: New and remeasured laboratory oscillator strengths for Mn I, the complete table is available online.
Table 2: Lines selected for solar abundance calculation. The NLTE abundances refer to MAFAGS-ODF (ODF) and Holweger & Müller (HM) model atmospheres. Van der Waals damping interaction constants $\log C_{\rm 6}$ are computed according to Anstee & O'Mara (1995); a correction of $\Delta\log C_{\rm 6} \approx -0.1$ is applied in order to fit the wings of strong lines.
Full version
Table 1: New and remeasured laboratory oscillator strengths for Mn I.