🌌✨ Using the U.S. National Science Foundation's Very Long Baseline Array (NSF VLBA), an international team led by Sergio A. Dzib (Max Planck Institute for Radio Astronomy) and co-led by Jazmín Ordoñez-Toro (Astronomical Observatory, Universidad de Nariño) has measured the dynamical masses of young binary stars in the Orion star-forming complex with sub-milliarcsecond precision. 📡🔭 By tracking the orbital motion of these tightly bound pairs at 5 GHz — a wavelength at which Orion's dense dust becomes transparent — the DYNAMO-VLBA program turns Orion into a precision laboratory for testing models of pre-main-sequence stellar evolution. The results, published in Astronomy & Astrophysics, reveal mismatches with standard models, hidden close companions, and persistent magnetic activity in surprisingly massive young stars.











