Table 4: Orbital solutions for FN Sgr.
Component K $\gamma_0$ e $\omega$ T01 $\Delta T^{2}$ $a \sin i$ f(M)
  [km s-1] [km s-1]   [deg] [JD 24...] [day] [AU] [$M_\odot $]
M giant $10.0\pm0.3$ $-53.4\pm0.2$ 03     2.2 0.52 0.0580
M giant $10.0\pm0.3$ $-53.4\pm0.2$ $0.06\pm0.03$ $368\pm29$ 50995 7.1 0.52 0.0586
cF-abs $22.0\pm1.5$ $-48.2\pm0.9$ 03   50718 -24.8 1.15 0.6300
cF-abs $23.3\pm1.0$ $-47.5\pm0.6$ $0.33\pm0.05$ $240\pm9$ 51614 -16.4 1.15 0.6259
He II wings $16.8\pm2.0$ $-51.3\pm1.2$ 03     29.0 0.88 0.2795
He II wings $18.3\pm1.4$ $-51.6\pm1.1$ $0.33\pm0.10$ $271\pm15$ 53424 26.8 0.90 0.3042
H$\alpha $+H$\beta $ wings $11.0\pm1.3$ $-51.2\pm0.8$ 03     -19.1 0.57 0.0783
Fe II $9.3\pm1.8$ $-60.0\pm1.8$ 03     -75.3 0.48 0.0468
He I $15.8\pm1.0$ $-54.1\pm0.8$ 03     -32.2 0.82 0.2310
He II $16.5\pm1.3$ $-53.8\pm0.8$ 03     -33.1 0.86 0.2656
[Fe VII]$\lambda $6087 $21.7\pm2.9$ $-66.2\pm1.8$ 03     95.2 1.13 0.6028
1 Time of the passage through periastron.
2 $\Delta T = T_{\rm sp~conj}-T_{\rm phot~ min}$.
3 Assumed.

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