Table 1: Overview of the used evolutionary models from D'Antona & Mazzitelli (1994) (DM94), D'Antona & Mazzitelli (1997) (DM97), BCAH98, PS99, Siess et al. (2000) (SDF00) and Yi et al. (2003) (YKD03) with the choices of free parameters. The table is restricted to those parameters which are necessary to distinguish between the models.
model metallicity Y X_D/10^-5 Convection

DM94 MLT

CM

DM97 Z=0.01 0.26 $2\times10^{-5}$

Z=0.01 0.26 $4\times10^{-5}$

Z=0.01 0.28 $1\times10^{-5}$

Z=0.01 0.28 $2\times10^{-5}$

Z=0.01 0.28 $4\times10^{-5}$

BCAH98 [M/H]=0.0 0.275 MLT ( $\alpha=1.0$ )

[M/H]=0.0 0.275 MLT ( $\alpha=1.5$ )

[M/H]=0.0 0.282 MLT ( $\alpha=1.9$ )

[M/H]=-0.5 0.250 MLT ( $\alpha=1.0$ )

PS99 0.28 MLT ( $\alpha=1.5$ )

SDF00 Z=0.01 0.256

Z=0.02 0.277

Z=0.02 0.277 +overshooting

Z=0.03 0.297

Z=0.04 0.318

YKD03 Z=0.01

Z=0.023

Z=0.03

**Table 1:** Overview of the used evolutionary models from D'Antona & Mazzitelli (1994) (DM94), D'Antona & Mazzitelli (1997) (DM97), BCAH98, PS99, Siess et al. (2000) (SDF00) and Yi et al. (2003) (YKD03) with the choices of free parameters. The table is restricted to those parameters which are necessary to distinguish between the models.
model	metallicity	Y	X_D/10^-5	Convection
DM94				MLT
				CM
DM97	Z=0.01	0.26	$2\times10^{-5}$
	Z=0.01	0.26	$4\times10^{-5}$
	Z=0.01	0.28	$1\times10^{-5}$
	Z=0.01	0.28	$2\times10^{-5}$
	Z=0.01	0.28	$4\times10^{-5}$
BCAH98	[M/H]=0.0	0.275		MLT ( $\alpha=1.0$ )
	[M/H]=0.0	0.275		MLT ( $\alpha=1.5$ )
	[M/H]=0.0	0.282		MLT ( $\alpha=1.9$ )
	[M/H]=-0.5	0.250		MLT ( $\alpha=1.0$ )
PS99		0.28		MLT ( $\alpha=1.5$ )
SDF00	Z=0.01	0.256
	Z=0.02	0.277
	Z=0.02	0.277		+overshooting
	Z=0.03	0.297
	Z=0.04	0.318
YKD03	Z=0.01
	Z=0.023
	Z=0.03

Source LaTeX | All tables | In the text

	1 Introduction
	2 A new method - extending the approach of White et al. (1999)
	3 Application to known eclipsing binaries
	4 Summary and conclusions
	References
	Online Material
	Appendix A: Derivation of intrinsic scale errors
	Appendix B: Conversion tables