Free Access
Issue
A&A
Volume 525, January 2011
Article Number A63
Number of page(s) 16
Section Stellar atmospheres
DOI https://doi.org/10.1051/0004-6361/200912356
Published online 01 December 2010

Online material

Table 4

Hyperfine structure for Mn i and Cu i lines.

Table 5

Signal to noise measured around λ6000 for stars analyzed here and in Allen & Barbuy (2006a).

Table 6

Data from the literature for stars that were analyzed in more than one work.


© ESO, 2010

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