The HD 98800 quadruple pre-main sequence system

ZÚÑIGA-FERNÁNDEZ, S.; OLOFSSON, J.; BAYO, A.; HAUBOIS, X.; CORRAL-SANTANA, J. M.; LOPERA-MEJÍA, A.; RONCO, M. P.; TOKOVININ, A.; GALLENNE, A.; KENNEDY, G. M.; BERGER, J.-P.

ASTRONOMY AND ASTROPHYSICS

EDP SCIENCES S A

Lugar: Paris; Año: 2021 vol. 655

0004-6361

Context. HD 98800 is a young (∼ 10 Myr old) and nearby (∼ 45 pc) quadruple system, composed of two spectroscopic binariesorbiting around each other (AaAb and BaBb), with a gas-rich disk in polar configuration around BaBb. While the orbital parametersof BaBb and AB are relatively well constrained, this is not the case for AaAb. A full characterisation of this quadruple system canprovide insights on the formation of such a complex system.Aims. The goal of this work is to determine the orbit of the AaAb subsystem and refine the orbital solution of BaBb using multi-epochinterferometric observations with the Very Large Telescope Interferometer (VLTI)/PIONIER and radial velocities.Methods. The PIONIER observations provide relative astrometric positions and flux ratios for both AaAa and BaBb subsystems.Combining the astrometric points with radial velocity measurements, we determine the orbital parameters of both subsystems.Results. We refined the orbital solution of BaBb and derived, for the first time, the full orbital solution of AaAb. We confirmedthe polar configuration of the circumbinary disk around BaBb. From our solutions, we also inferred the dynamical masses of AaAb(MAa = 0.93 ±0.09 and MAb = 0.29 ±0.02 M ). We also revisited the parameters of the AB outer orbit.Conclusions. The orbital parameters are relevant to test the long-term stability of the system and to evaluate possible formationscenarios of HD 98800. Using the N-body simulation, we show that the system should be dynamically stable over thousands of orbitalperiods and that it made preliminary predictions for the transit of the disk in front of AaAb which is estimated to start around 2026.We discuss the lack of a disk around AaAb, which can be explained by the larger X-ray luminosity of AaAb, promoting faster photo-evaporation of the disk. High-resolution infrared spectroscopic observations would provide radial velocities of Aa and Ab (blendedlines in contemporary observations), which would allow us to calculate the dynamical masses of Aa and Ab independently of theparallax of BaBb. Further monitoring of other hierarchical systems will improve our understanding of the formation and dynamicalevolution of these kinds of systems.