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Table 3
The Mn i abundances determined from the best fits to the solar spectrum.
Mn i line (approx. Å) | log N(Mn) |
|
|
12 899 | −6.54 |
12 975 | −6.54 |
13 281 | −6.64 |
13 293 | −6.64 |
13 318 | −6.54 |
13 415 | −6.54 |
Notes. The uncertainty in the log N(Mn) values is ± 0.05 and relates to the step size in the grid of manganese abundances.
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