The most metal-poor quadruple system of subdwarfs G89-14

The system of subdwarfs G89-14 is one of the most metal-poor multiple stars with an atmospheric metal abundance [ m/H] = -1.9. Speckle interferometry at the 6-m BTA telescope has revealed that G89-14 consists of four components. Measurements of the magnitude difference between the components and published data have allowed their masses to be estimated: M _A ≈ 0.67 M _⊙, M _B ≈ 0.24 M _⊙, M _C ≈ 0.33 M _⊙, and M _D ≈ 0.22 M _⊙. The ratio of the orbital periods of the subsystems has been obtained, 0.52 yr: 3000 yr: 650 000 yr (1: 5769: 1 250 000), indicative of a high degree of hierarchy o fG89-14 and its internal dynamical stability. The calculated Galactic orbital elements and the low metallicity of the quadruple system suggest that it belongs to the Galactic halo.