Beryllium abundances and star formation in the halo and in the thick disk

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Volume 499 / No 1 (May III 2009)

A&A, 499 1 (2009) 103-119

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Table 9:

A comparison of the linear relations between Be and Fe and O (or any other $\alpha$ indicators adopted) as found in the literature.
$\log$ (Be/H) = (A $\pm$ $\sigma_{A}$ ) + (B $\pm$ $\sigma_{B}$ ) [Fe/H]	Ref.
$\log$ (Be/H) = (- $10.38 \pm 0.08$ ) + ( $1.24 \pm 0.07$ ) [Fe/H]	This work (all stars)
$\log$ (Be/H) = (- $10.34 \pm 0.09$ ) + ( $1.27 \pm 0.08$ ) [Fe/H]	This work (F00 stars)
$\log$ (Be/H) = (- $10.40 \pm 0.08$ ) + ( $1.22 \pm 0.07$ ) [Fe/H]	This work (halo stars)
$\log$ (Be/H) = (- $10.38 \pm 0.08$ ) + ( $1.16 \pm 0.07$ ) [Fe/H]	This work (thick disk stars)
$\log$ (Be/H) = (- $10.22 \pm 0.07$ ) + ( $1.16 \pm 0.04$ ) [Fe/H]	King (2001)
$\log$ (Be/H) = (- $10.59 \pm 0.03$ ) + ( $0.96 \pm 0.04$ ) [Fe/H]	Boesgaard et al. (1999)
$\log$ (Be/H) = (- $10.19 \pm 0.11$ ) + ( $1.07 \pm 0.08$ ) [Fe/H]	Molaro et al. (1997a)
$\log$ (Be/H) = (- $9.76 \pm 0.22$ ) + ( $1.26 \pm 0.11$ ) [Fe/H]	Boesgaard & King (1993)
$\log$ (Be/H) = (- $10.87 \pm 0.51$ ) + ( $0.77 \pm 0.23$ ) [Fe/H]	Gilmore et al. (1992)²
$\log$ (Be/H) = (A $\pm$ $\sigma_{\rm A}$ ) + (B $\pm$ $\sigma_{\rm B}$ ) [ $\alpha$ /H]	Ref.
$\log$ (Be/H) = (- $10.62 \pm 0.07$ ) + ( $1.36 \pm 0.08$ ) [ $\alpha$ /H]	This work (all stars)
$\log$ (Be/H) = (- $10.71 \pm 0.07$ ) + ( $1.34 \pm 0.08$ ) [ $\alpha$ /H]	This work (F00 stars)
$\log$ (Be/H) = (- $10.62 \pm 0.07$ ) + ( $1.37 \pm 0.08$ ) [ $\alpha$ /H]	This work (halo stars)
$\log$ (Be/H) = (- $10.64 \pm 0.07$ ) + ( $1.31 \pm 0.08$ ) [ $\alpha$ /H]	This work (thick disk stars)
$\log$ (Be/H) = (- $10.87 \pm 0.28$ ) + ( $1.10 \pm 0.18$ ) [Mg/H]	King (2002)
$\log$ (Be/H) = (- $10.33 \pm 0.16$ ) + ( $1.31 \pm 0.18$ ) [Ca/H]	King (2002)
$\log$ (Be/H) = (- $10.61 \pm 0.06$ ) + ( $1.51 \pm 0.05$ ) [O/H] $^{1}_{\rm mean}$	King (2001)
$\log$ (Be/H) = (- $10.69\pm 0.04$ ) + ( $1.45 \pm 0.04$ ) [O/H]	Boesgaard et al. (1999)
$\log$ (Be/H) = (- $10.62 \pm 0.13$ ) + ( $1.13 \pm 0.11$ ) [O/H]	Molaro et al. (1997a)
$\log$ (Be/H) = -10.68 + 1.12 [O/H]	Boesgaard & King (1993)
$\log$ (Be/H) = (- $11.19 \pm 0.25$ ) + ( $0.85 \pm 0.15$ ) [O/H]	Gilmore et al. (1992)²

¹ A mean oxygen abundance from different indicators, such as the molecular OH UV lines and the $\lambda$ 6300 [OI] forbidden line; ² the fits were recalculated in this work based on the original published data.

Source LaTeX | All tables | In the text

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