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Table 3.

Orbital, photometric, and absolute physical parameters of the three studied eclipsing binaries.

Parameter ASAS-052 A ASAS-065 ASAS-073
P (d) 5.2735660(9) 8.219626(13) 1.446253(2)
T0 [JD-2450000] 1873.2045(7) 1883.320(2) 1870.166(2)
Tp [JD-2450000] 2874.920(4) 1887.92(6) 1869.803(2)
K1 (km s−1) 53.8(3) 51.32(4) 88.3(5)
K2 (km s−1) 91.9(2.3) 72.84(4) 158.6(1.6)
q 0.586(15) 0.705(4) 0.556(6)
e 0.145(5) 0.0113(7) 0.0(fix)
ω (°) 66(2) 291(3)
γ1 (km s−1) 19.8(7) 10.36(4) 35.1(4)
γ2 − γ1 (km s−1) −3(7) 0.3(4) 2.8(1.4)
1sin3i (M) 1.03(6) 0.956(12) 1.448(34)
2sin3i (M) 0.60(2) 0.674(5) 0.806(13)
a sin i (R) 15.03(24) 20.18(7) 7.06(5)
rmsRV, 1 (km s−1)a 0.105/0.114 0.019/0.100 1.00/1.35
rmsRV, 2 (km s−1)a –/1.24 0.255/1.168 4.09/4.54
i (°) 88.94(5) 89.66(2) 87.91(1)
r1 0.0682(6) 0.0494(1) 0.2314(6)
r2 0.0390(13) 0.0342(3) 0.1160(14)
Ω1 15.24(12) 20.93(4) 4.866(4)
Ω2 16.22(13) 21.73(7) 6.016(5)
Teff, 2/Teff, 1 b 0.697(2) 0.722(1) 0.6835(6)
(l2/l1)ASAS V 0.018(12) 0.06(5) 0.032(6)
  ASAS I 0.060(14)
  MITSuME g 0.032(5) 0.0294(5)
  MITSuME R 0.020(2) 0.086(5) 0.0467(2)
  MITSuME I 0.054(4) 0.136(5) 0.0604(3)
(l3)ASAS V 0.44(3) 0.09(4)
  MITSuME g 0.084(4)
  MITSuME R 0.41(2) 0.092(4)
  MITSuME I 0.41(2) 0.010(4)
rmsASAS V (mag) 0.021 0.018 0.015
  ASAS I (mag) 0.021
  MITSuME g (mag) 0.019 0.016
  MITSuME R (mag) 0.015 0.016 0.013
  MITSuME I (mag) 0.017 0.016 0.015
1 (M) 1.03(6) 0.956(12) 1.452(34)
2 (M) 0.60(2) 0.674(5) 0.808(13)
a (R) 15.03(24) 20.18(7) 7.06(5)
R1 (R) 1.03(2) 0.997(4) 1.635(12)
R2 (R) 0.59(2) 0.690(7) 0.819(11)
log(g1) 4.430(14) 4.421(3) 4.173(5)
log(g2) 4.684(28) 4.589(9) 4.519(10)
vsyn, 1 (km s−1) 9.8(2) 6.14(3) 57.2(4)
vsyn, 2 (km s−1) 5.6(2) 4.25(5) 28.7(4)
log(τsyn) (yr) 7.152(14) 7.825(3) 4.932(6)
log(τcir) (yr) 9.194(8) 10.276(2) 6.183(3)
Teff, 1 (K)c 5300(340) 5500(100) 6400(100)
Teff, 2 (K)c 3700(230) 3970(110) 4370(110)
log(L1/L) −0.13(11) −0.09(3) 0.60(3)
log(L2/L) −1.24(11) −0.96(5) −0.66(5)
[Fe/H] +0.5d +0.09(13) −0.27(8)
d (pc)e 102(14) 108(10) 170(5)

Notes.

(a)

Without and with IRCS.

(b)

Obtained with PHOEBE.

(c)

From various sources, see text for details.

(d)

Assumed.

(e)

Without extinction.

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