New simulations show that magnetic field interactions can decrease the distance between still-forming binary protostars. These results can help explain the characteristics of the binary star systems observed in the Milky Way. The results can also be extrapolated to binary black holes, giving insights into how supermassive black holes evolve. The work is published in the journal Monthly Notices of the Royal Astronomical Society.
Stars form from clouds of interstellar gas that collapse into dense regions known as molecular cloud cores. Multiple stars form close together simultaneously, and in some cases, two stars will become gravitationally bound to each other, forming a binary star system.
Credit: Third Party Reference
Observations suggest that these binary systems form early on, before the stars are even fully formed. Astronomers have struggled to explain how these still-forming “protostars” can pull together into binary systems so quickly.
The simulations using the ATERUI III and ATERUI II supercomputers at the National Astronomical Observatory of Japan have shown that interactions between an interstellar magnetic field and the gas around the protostars can remove angular momentum from the protostar pair, allowing the binary systems to form within a realistic time period.
In the simulation run with zero magnetic field performed as part of this research, the protostars actually moved farther apart, indicating the importance of the magnetic field in the process.
Credit: Third Party Reference
The simulations also suggest that the same process could work on massive binary black holes in the gas-rich heart of a new galaxy formed from the merger of two smaller galaxies. This would help explain how massive black holes can move close enough to merge and form a supermassive black hole.
Direct simulation of massive binary black holes over the timespans required to spiral toward each other is still computationally challenging, so rigorous investigation of the effects of magnetic fields on massive binary black holes remains a topic for future investigation.
Reference: https://phys.org/news/2026-06-magnetic-field-binary-star-simulations.html
