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Table 1.

Orbital and physical parameters and uncertainties of the binary system and its component stars.

Parameters of the binary system
Orbital period P [d] 221 ± 1
Eccentricity e 0.52 ± 0.03
Mass ratio q = M B M Be $ q = \nicefrac{M_{\mathrm{B}}}{M_{\mathrm{Be}}} $
– evolutionary q evol = M B , evol M Be , dyn $ q_{\mathrm{evol}}= \nicefrac{M_{\mathrm{B, evol}}}{M_{\mathrm{Be, dyn}}} $ ≤0.14
– spectroscopic q spec = M B , spec M Be , dyn $ q_{\mathrm{spec}}=\nicefrac{M_{\mathrm{B, spec}}}{M_{\mathrm{Be, dyn}}} $ ≤0.10
– dynamic q dyn = K Be K B $ q_{\mathrm{dyn}}=\nicefrac{K_{\mathrm{Be}}}{K_{\mathrm{B}}} $ 0.066 ± 0.053
Barycentric velocity v0 [km s−1] 62.3 ± 1.0
Distance d [pc] 1730 ± 260
Parameters of B star
Effective temperature Teff,B [kK] 13.5 ± 0.5
Surface gravity log(gB/cm s−2) 2.25 ± 0.25
Rotation velocity vrot, Bsini [km s−1] ≤30
Macroturbulent velocity vmac,B [km s−1] ≤50
Microturbulent velocity vmic,B [km s−1] 10.0 (fixed)
Continuum flux ratio fB/ftot(4300 Å) 0.60 ± 0.08
Radius RB [R] 9 . 0 1.7 + 2.1 $ 9.0^{+2.1}_{-1.7} $
Bolometric luminosity LB [L] 2300 800 + 1300 $ 2300^{+1300}_{-800} $
Spectroscopic mass MB, spec [M] 0 . 69 0.31 + 0.63 $ 0.69^{+0.63}_{-0.31} $
Evolutionary mass MB, evol [M] 0.99 ± 0.11
RV semi-amplitude KB [km s−1]
– orbit model 74.1 ± 2.2
– disentangling 76.0 ± 0.9
Parameters of the Be star
Effective temperature Teff,Be [kK] 17 1 + 2 $ 17^{+2}_{-1} $
Surface gravity log(gBe/cm s−2) 4.0 ± 0.5
Rotation velocity vrot, Besini [km s−1] 270 ± 70
Macroturbulent velocity vmac,Be [km s−1] 50 (fixed)
Microturbulent velocity vmic,Be [km s−1] 2 (fixed)
Continuum flux ratio fBe/ftot(4300 Å) 0.40 ± 0.08
Radius RBe [R] 6 . 0 1.3 + 1.6 $ 6.0^{+1.6}_{-1.3} $
Bolometric luminosity LBe [L] 2700 1100 + 1600 $ 2700^{+1600}_{-1100} $
Spectroscopic mass MBe, spec [M] 10 . 5 7.1 + 21.5 $ 10.5^{+21.5}_{-7.1} $
Evolutionary mass MBe, evol [M] 6.5 ± 0.9
Min. dynamic mass MBe, dyn [M] ≥7.0
RV semi-amplitude KBe [km s−1] 5 ± 4

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