Absolute dimensions of solar-type eclipsing binaries - II. V636 Centauri: A 1.05 primary with an active, cool, oversize 0.85 secondary

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Table 4:

Adopted photometric elements for V636 Cen.
i	$89{\hbox{$.\!\!^\circ$ }}65 \pm 0{\hbox{$.\!\!^\circ$ }}10$
$r_{\rm p}$	$0.0740 \pm 0.0003$
$r_{\rm s}$	$0.0603 \pm 0.0003$

	y	b	v	u
$L_{\rm s}/L_{\rm p}$	0.269	0.237	0.178	0.152
	$\pm$ 15	$\pm$ 15	$\pm$ 15	$\pm$ 15

Note: The individual luminosity ratios are based on the mean stellar and orbital
parameters and include the average activity level (spots) in 1987 and 1988.

Source LaTeX | All tables | In the text

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