The universality of the relation between magnetic fields and star formation in galaxies
Davide Belfiori, Sergio Martin-Alvarez, Enrique Lopez-Rodriguez, Rosita Paladino

TL;DR
This study demonstrates a near-universal relation between magnetic field strength and star formation rate across diverse galaxy types, supporting supernova-driven turbulence as the key amplification mechanism.
Contribution
It provides the first comprehensive analysis confirming the universal magnetic field–star formation relation across galaxy properties and ISM phases using cosmological simulations.
Findings
Magnetic field strength scales with star formation rate with a slope of approximately 0.2-0.3.
The $B$-$ ext{SFR}$ relation supports supernova-driven turbulence as the origin.
Simulated trends align with observations, confirming turbulence as the main amplification process.
Abstract
The interstellar medium (ISM) is permeated by magnetic fields that affect gas dynamics and star formation. These fields correlate with supernova (SN)-driven turbulence, but whether the scaling is universal across galaxy properties, ISM phases, and energy budgets remains unclear. We quantify the dependence of magnetic fields on star formation activity including both regular and starburst galaxies. We analyse 19 spiral disks from the cosmological RTnsCRiMHD Azahar suite, deriving line-of-sight integrated maps to measure median magnetic-field strength (), specific energies (thermal, turbulent, magnetic, and cosmic-ray), and star formation rate (SFR), star formation surface density () and specific SFR (sSFR). We find an almost universal magnetic-field-SFR scaling with slope - across galaxy mass and ISM phases. The…
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