Structure and spectra of irradiated secondaries in close binaries - A model calculation of the pre-cataclysmic variable UU Sagittae | A&A

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Table 4:

Final results (see discussion):
	Primary	Secondary
$T_{{\rm eff}}$	80 000 to 85 000 K	(6000 to 7000 K)
$T_{\rm eq}$	n.a.	24 000 to 26 000 K
$\log g$	(4.5), 5.0 to 5.2	(4.45)
$\epsilon_{{\rm He}}$	-0.2 to -0.4 dex	n.a.
$\epsilon_{{\rm C}}$	-0.2 dex	+1.0 to +1.5 dex
$\epsilon_{{\rm N}}$	+1.2 dex and more	$\approx$ +1.0 dex
$L = 4\pi\sigma r^2 T_{{\rm eff}}^4$	1 to $2\times 10^{37}$ erg s^-1	1 to $3 \times 10^{33}$ erg s^-1
$L = 4\pi\sigma r^2 T_{{\rm eq}}^4$	n.a.	2 to $5\times 10^{35}$ erg s^-1

Source LaTeX | All tables | In the text