Low-metallicity star formation: Relative impact of metals and magnetic fields

TL;DR

This study investigates how metals and magnetic fields influence low-metallicity star formation, revealing that magnetic fields stabilize protostellar discs and significantly affect fragmentation and timescales, with implications for early star formation.

Contribution

It provides a comprehensive analysis of the relative roles of metals and magnetic fields in low-metallicity star formation, highlighting magnetic fields' stabilizing effects and their impact on fragmentation processes.

Findings

Magnetic fields stabilize protostellar discs and reduce fragmentation.

Fragmentation timescale decreases without magnetic fields at Z>0.

Magnetic fields increase fragmentation timescale by a factor of about 3.

Abstract

Low-metallicity star formation poses a central problem of cosmology, as it determines the characteristic mass scale and distribution for the first and second generations of stars forming in our Universe. Here, we present a comprehensive investigation assessing the relative impact of metals and magnetic fields, which may both be present during low-metallicity star formation. We show that the presence of magnetic fields generated via the small-scale dynamo stabilises the protostellar disc and provides some degree of support against fragmentation. In the absence of magnetic fields, the fragmentation timescale in our model decreases by a factor of ~10 at the transition from Z=0 to Z>0, with subsequently only a weak dependence on metallicity. Similarly, the accretion timescale of the cluster is set by the large-scale dynamics rather than the local thermodynamics. In the presence of magnetic fields, the primordial disc can become completely stable, therefore forming only one central fragment. At Z>0, the number of fragments is somewhat reduced in the presence of magnetic fields, though the shape of the mass spectrum is not strongly affected in the limits of the statistical uncertainties. The fragmentation timescale, however, increases by roughly a factor of 3 in the presence of magnetic fields. Indeed, our results indicate comparable fragmentation timescales in primordial runs without magnetic fields and Z>0 runs with magnetic fields.