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Table 5

Stellar abundances of Mo and Ru for dwarf stars.

Dwarfs T log g ξ [Fe/H] [Mo/Fe] [Mo/Fe] [Ru/Fe]
[K] [km s-1] (3864A) (5506A)
BD+09 2190 6450a 4.00 1.5 −2.60 ... ... ...
BD-13 3442 6450 4.20a 1.5 −2.56 ... ... ...
CD-30 18140 6340 4.13 1.0 −1.92 ... ... <0.7
CD-33 3337 5952 3.95 1.4 −1.55 ... ... 0.56
CD-45 3283 5657c 4.97 0.8 −0.99 0.31 <0.25 0.55
CD-57 1633 5907 4.26 1.1 −1.01 ... ... 0.40+
HD 3567 6035 4.08 1.5 −1.33 0.50 ... 0.74
HD 19445 5982 4.38 1.4 −2.13 ... ... 0.70
HD 22879 5792 4.29 1.2 −0.95 ... ... 0.43
HD 25704 5700 4.18 1.0 −1.12 0.20 ... 0.22
HD 63077 5629 4.15 0.9 −1.05 0.30 ... 0.35
HD 63598 5680 4.16 0.9 −0.99 ... <0.0 0.33
HD 76932 5905 4.08 1.3 −0.97 0.45 ... 0.53
HD 103723 6128 4.28 1.5 −0.85 0.45 ... 0.45
HD 105004 5900a 4.30c 1.1 −0.84 <0.35 ... 0.37
HD 106038b 5950 4.33 1.1 −1.48 0.70 ... 0.75
HD 111980b 5653 3.90 1.2 −1.31 0.51 <0.5 0.52
HD 113679 5759 4.04 0.9 −0.63 0.22 0.2 0.35
HD 116064 5999 4.33 1.5 −2.19 ... ... <1.05
HD 120559 5411 4.75 0.7 −1.33 0.75 ... 0.75
HD 121004 5711 4.46 0.7 −0.73 ... 0.3 0.55
HD 122196 6048 3.89 1.2 −1.81 ... ... 0.47
HD 126681b 5532 4.58 0.6 −1.28 0.62 0.6 0.71
HD 132475 5838 3.90 1.5 −1.52 0.64 ... 0.73
HD 140283 5738 3.73 1.3 −2.58 ... ... ...
HD 160617 6028 3.79 1.3 −1.83 ... ... 0.85
HD 166913 6155 4.07 1.5 −1.30 0.43 ... 0.55
HD 175179 5758 4.16 0.9 −0.72 0.4cp <0.3 0.37
HD 188510 5536 4.63 1.0 −1.58 0.40 ... 0.54
HD 189558 5712 3.79 1.2 −1.18 0.54 <0.68 0.59
HD 195633 6005 3.86 1.4 −0.71 ... ... 0.08
HD 205650 5842 4.49 0.9 −1.19 0.48 ... 0.52
HD 213657 6208 3.78 1.2 −2.01 ... ... ...
HD 298986 6144 4.18 1.4 −1.48 0.50 ... 0.66
G005-040 5766 4.23a 0.8 −0.93 0.30 <0.35 0.39
G013-009 6416 3.95 1.4 −2.27 ... ... ...
G020-024 6482 4.47 1.5 −1.89 ... ... <1.0
G064-012 6459 4.31c 1.5 −3.10 ... ... ...
G064-037 6494 3.82c 1.4 −3.17 ... ... ...
G088-032 6327 3.65 1.5 −2.50 ... ... ...
G088-040 5929 4.14 1.4 −0.90 0.18 ... 0.30
G183-011 6309 3.97 1.0 −2.12 ... ... ...

Notes.

(+)

Larger uncertainty in the abundance due to blends.

(cp)

Continuum placement uncertain.

(a)

T is derived from excitation potentials, log g from ionisation equilibrium;

(b)

the star has a special r-process pattern;

(c)

uncertain colour, dereddening, or parallax lead to adjustment according to note (a).

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