On the role of magnetic fields in abundance determinations
J. M. Borrero

TL;DR
This study quantifies how magnetic fields in stellar atmospheres can bias elemental abundance measurements, especially for iron, and provides a model to assess when magnetic effects are significant.
Contribution
The paper introduces a simulation-based analysis of magnetic field impacts on spectral line formation and abundance determination, highlighting the importance of magnetic inclination and proposing a practical assessment model.
Findings
Iron abundance can be biased by up to 0.1 dex due to magnetic fields.
Magnetic effects on Si, C, O are negligible (<0.02 dex).
Magnetic inclination significantly influences abundance bias.
Abstract
{Although there is considerable evidence supporting an ubiquitous magnetic field in solar/stellar photospheres, its impact in the determination of abundances has never been quantified. In this work we investigate whether the magnetic field plays a measurable role for this kind of studies. To that end, we carry out simulations of spectral line formation in the presence of a magnetic field, and then use those profiles to derive the abundance of several atomic species (Fe, Si, C and O) neglecting the magnetic field. In this way, we find that the derived iron abundance can be significantly biased, with systematic errors up to 0.1 dex. In the case of silicon, carbon and oxygen their role is very marginal (errors smaller than 0.02 dex). We also find that the effect of the magnetic field strongly depends on its inclination with respect to the observer. We show that fields that are aligned with…
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