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Table 10

High-resolution average Hyades abundances from giants.

Here S09/S06a Bo00b V99c

R = λ/δλ 30 000 60 000 45 000 30–65 000
S/N 50–100 100–200 100–300  ~200

 [Fe/H]  +0.11  ±  0.01 +0.21  ±  0.04 +0.12  ±  0.06 –0.05  ±  0.03
 [Al/Fe]  +0.00  ±  0.02 +0.17  ±  0.03 +0.13  ±  0.06
 [Ba/Fe]  +0.36  ±  0.04 +0.10  ±  0.03 –0.03  ±  0.07
 [Ca/Fe]  –0.07  ±  0.01 +0.03  ±  0.05 +0.03  ±  0.04
 [Co/Fe]  +0.03  ±  0.03 +0.00  ±  0.02
 [Cr/Fe]  +0.04  ±  0.03 –0.02  ±  0.02
 [La/Fe]  –0.08  ±  0.04 –0.10  ±  0.08
 [Mg/Fe]  +0.10  ±  0.08 +0.38  ±  0.03 +0.16  ±  0.01 +0.17  ±  0.04
 [Na/Fe]  +0.18  ±  0.01 +0.45  ±  0.04 +0.37  ±  0.05 +0.10  ±  0.05
 [Ni/Fe]  +0.03  ±  0.01 +0.05  ±  0.07 +0.05  ±  0.06 +0.04  ±  0.04
 [O/Fe]  –0.27  ±  0.04 –0.08  ±  0.05 +0.11  ±  0.04
 [Sc/Fe]  –0.02  ±  0.02 +0.00  ±  0.01 +0.03  ±  0.07
 [Si/Fe]  +0.09  ±  0.01 +0.07  ±  0.01 +0.13  ±  0.03
 [Ti/Fe]  –0.09  ±  0.04 –0.04  ±  0.02
 [V/Fe]  +0.04  ±  0.05 –0.01  ±  0.03
 [Y/Fe]  –0.09  ±  0.03 –0.04  ±  0.02 –0.04  ±  0.07

References. 

(a)

Schuler et al. (2009) and Schuler et al. (2006), from the same 3 K giants studied here.

(b)

Boyarchuk et al. (2000), from the same 3 K giants studied here.

(c)

Varenne & Monier (1999), from 29 F dwarfs.

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