RMHD simulations with stellar mass loading produce parsec-scale radio-optical offsets only in the jet power range 10^42.5-10^44 erg/s, linking offsets to stellar evolution and providing a jet power diagnostic.
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Stellar mass loading drives dissipation and reacceleration in AGN jets: Explaining VLBI-Gaia offsets and constraining jet power
RMHD simulations with stellar mass loading produce parsec-scale radio-optical offsets only in the jet power range 10^42.5-10^44 erg/s, linking offsets to stellar evolution and providing a jet power diagnostic.