Abstract

Our knowledge about the multiplicity of intermediate mass A- and B-type stars is still incomplete, in particular for high (3+) multiplicity systems. Here we report the discovery of a new companion to the nearby roAp star HIP 47145 = HR 3831 with a K band flux ratio of 4% based on a VLTI/GRAVITY interferometric observation. This new 0.64M ⊙ companion at a projected separation 187.5 mas ↔ 13.40 au explains the Hipparcos-GaiaDR2 proper motion change of HR 3831. Together with the previously known M ≈ 1M ⊙ companion at 3″ ↔ 214 au, this makes HR 3831 a hierarchical triple and a very likely progenitor for a system similar to 40 Eridani.

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