Abstract
Abstract
2 Hydrae is a nearby M
Aa = 1.66M
⊙
δ Scuti star with strong astrometric evidence for a close companion in addition to its known M
B
= 0.20M
⊙ M dwarf companion at 530 au. Here we report on a VLTI/GRAVITY near-infrared interferometric observation that reveals the close companion to be a M
Ab = 1.18M
⊙ star at a projected separation ρ = 168 mas ↔ 8.4 au. This triple system is a potential progenitor for a double white dwarf binary under the dynamical influence of an outer M dwarf companion with a low enough hierarchy for potentially interesting dynamical effects.
Publisher
American Astronomical Society