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 $[\mathrm{m}\mathrm{/}\mathrm{H}]=-1.9$. 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: $M_A\approx 0.67M_{\odot }$, $M_B\approx 0.24M_{\odot }$, $M_{C}\approx0.33 M_{\odot}$,and$M_{D}\approx0.22 M_{\odot}$. The ratio of the orbital periods of the subsystems has been obtained, 0.52 yr : 3 000 yr : 650 000 yr (1:5769:1250000), indicative of a high degree of hierarchy of G89-14 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.