Two-σ lower limits on fundamental parameters of the binary system, as derived from the combination of interferometric and radial velocity data.
|Mass of the primary star M1 (M⊙)||0.75|
|Mass of the secondary star M2 (M⊙)||1.65|
|Separation a (au)||1.74|
|Luminosity of the primary star L1 (L⊙)||14 000|
|Radius of the primary star R1 (R⊙)||75|
|Distance d (kpc)||1.4|
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