Table 2
Adopted abundances for the Sun, Arcturus, and μ Leo.
| El. | Z | log ϵ(X) | ||||||||
|
|
||||||||||
| Sun | Arcturus | μ Leo | ||||||||
|
|
|
|
||||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | ||||
|
|
||||||||||
| Fe | 26 | 7.67 | 7.50 | 7.50 | 7.46 | 6.98 | 6.95 | 7.80 | ||
| Zn | 30 | 4.60 | 4.60 | 4.56 | 4.65 | 4.26 | 4.06 | 4.80 | ||
Notes. Solar abundances are from (1): Anders & Grevesse (1989); (2): Grevesse & Sauval (1998) (adopted); (3): Asplund et al. (2009); (4): Lodders et al. (2009); Arcturus abundances are from (5) Ramírez & Allende Prieto (2011); and (6) present fits, computed with parameters from Meléndez et al. (2003) (adopted abundances); μ Leo abundances are from (7) Lecureur et al. (2007), with Zn abundance of [Zn/Fe] = −0.1, or ϵ(Zn) = 4.80 derived here.
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