Table 3: Solar abundances and typical galactic depletion values ofelements investigated in this paper.
Ion log(X/H)+12a   [X/S]b,c  
    Cold disc Warm disc Halo
H  I 12.00 ... ... ...
Si  II $7.55\pm 0.02$ -1.3 -0.4 -0.3
S  II $7.27\pm 0.05$ +0.0 +0.0 +0.0
Cr  II $5.68\pm 0.03$ -2.1 -1.2 -0.6
Mn  II $5.53\pm 0.04$ -1.5 -1.0 -0.7
Fe  II $7.51\pm 0.01$ -2.2 -1.4 -0.6
Ni  II $6.25\pm 0.02$ -2.2 -1.4 -0.6
Zn  II $4.65\pm 0.02$ -0.4 -0.2 -0.1
a Solar and Meteorite abundances from Anders (1993).
b $[X/{\rm H]}= \log[Z(X)]-\log[Z_\odot(X)]$.
c Galactic values are from Welty et al. (1999).


Source LaTeX | All tables | In the text