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Table 3

Information for DN Cas and comparison of results between this work and Bakış et al. (2016).

G3$G_3^\prime $ (mag) 9.6799(54)
GBP,3GRP,3 (mag) 1.0113
ϖc (mas) 0.506(24)
d (kpc) 1.9930.090+0.099$1.993_{ - 0.090}^{ + 0.099}$

This work Bakış et al. (2016)

PHOEBE type Detached Detached
P(d) 2.31095(7) 2.310951(1)
Third light 0 (fix) 0
i(°) 79.2(20) 77.2(2)
sma (R) 23.8(2) 23.53(5)
Teff 1 (kK) 32.6(6) 32.1(10)
Teff 2 (kK) 29.6(7) 28.2(11)
M1 (M) 19.55(39) 19.04(7)
M2 (M) 14.15(28) 13.73(5)
R1 (R) 7.5(1) 7.22(6)
R2 (R) 4.82(9) 5.79(6)
f1 0.58(9) –0.10(7)
f2 –2.53(9) –0.22(9)

T0 (d) 2456901.9923(5) 2456287.2699
ω (°) 90 (fix) 90 (fix)
e 0 (fix) 0 (fix)
γ1 (km/s) –47.40(28) –45.5(3)
γ2 (km/s) –47.68(28) –45.5(3)
Κ1 (km/s) 214.60(40) 211(3)
K2 (km/s) 296.35(34) 292(5)
q 0.7242(16) 0.722(2)

Sp. class 1 O8.5 V(n) B0 V
Sp. class 1 B0 V Bl V
Β flux fr. 1 75%
Β flux fr. 2 25%

Notes. T0 is the heliocentric lulian date.

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