2025MNRAS.540.2830O

We present dynamical mass measurements, obtained from multi-epoch Very Long Baseline Interferometry (VLBI) observations, for the young multiple stellar system EC 95, located in the core of the Serpens star-forming region. Our data set includes both archival data and more recent observations obtained as part of the Dynamical Masses of Young Stellar Multiple Systems with the VLBA project (DYNAMO-VLBA), totalling 32 epochs over 12 yr of observation. The observations span more than half of the EC 95AB orbit, which has an estimated period of $21.6\pm 0.1$ yr, and yield masses of $2.15\pm 0.10$ M$_\odot$ for EC 95A and $2.00\pm 0.12$ M$_\odot$ for EC 95B. Furthermore, for the first time, we have estimated the mass of the third component (EC 95C) using four available radio detections as well as an infrared observation. We find it to be 0.26 $^{+0.53}_{-0.46}$ M$_\odot$, suggesting that E 95C is a low-mass T Tauri star. We conclude that EC 95 is a hierarchical triple system comprised of a tight central binary proto-Herbig AeBe system and a lower mass companion on a wider orbit. These results contribute to improve our understanding of the stellar dynamics in this system and provide valuable insights into its triple nature.