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Table 3

Best lightcurve solution of ASAS 10232.

Fixed parameters:

q(= M2 / M1) 0.34
Teff(1) [K] 28 400
g 1 b 1.0
g 2 b 0.32
x1(B)c 0.26
x1(V)c 0.22
x1(I)c 0.165
x1(white)c 0.20
δ 2 d 0.0
l 3 f 0.0

Adjusted parameters:
i [°] 65.86 ± 0.69
Teff(2) [K] 3380 ± 561
A 1 a 0.94 ± 0.03
A 2 a 1.21 ± 0.13
Ω1f 5.700 ± 0.260
Ω2f 2.673 ± 0.052
g 0.99954 ± 0.00077
g 0.99804 ± 0.00247
g 0.99036 ± 0.00845
g 0.99709 ± 0.00337
δ 1 0.0123 ± 0.0080
x2(B) 0.638 ± 0.097
x2(V) 0.548 ± 0.0630
x2(I) 0.625 ± 0.087
x2(white) 0.238 ± 0.089

Roche radiih:
r1(pole) [a] 0.184 ± 0.009
r1(point) [a] 0.186 ± 0.00
r1(side) [a] 0.185 ± 0.009
r1(back) [a] 0.186 ± 0.009
r2(pole) [a] 0.248 ± 0.009
r2(point) [a] 0.286 ± 0.017
r2(side) [a] 0.256 ± 0.010
r2(back) [a] 0.277 ± 0.014

Notes. 

(a)

Bolometric albedo.

(b)

Gravitational darkening exponent.

(c)

Linear limb darkening coefficient; taken from Wade & Rucinski (1985).

(d)

Radiation pressure parameter, see Drechsel et al. (1995).

(e)

Fraction of third light at maximum.

(f)

Roche potentials.

(g)

Relative luminosity; L2 is not independently adjusted, but recomputed from r2 and Teff(2).

(h)

Fractional Roche radii in units of separation of mass centers.

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