HARPS spectropolarimetry of three sharp-lined Herbig Ae stars: New insights

TL;DR

This study uses high-resolution spectropolarimetry to investigate magnetic fields in three Herbig Ae stars, revealing complex magnetic behaviors influenced by circumstellar matter and elemental inhomogeneities, with some stars showing detectable or variable fields.

Contribution

It provides new magnetic field measurements of three Herbig Ae stars using archival HARPS data, highlighting the effects of circumstellar matter and elemental inhomogeneities on magnetic field detection.

Findings

HD101412 shows differences in magnetic measurements depending on line lists.

HD104237's secondary T Tauri star has a strong magnetic field of 129G.

HD190073 exhibits a variable magnetic field influenced by circumstellar environment.

Abstract

Several arguments have been presented that favour a scenario in which the low detection rate of magnetic fields in Herbig Ae stars can be explained by the weakness of these fields and rather large measurement uncertainties. Spectropolarimetric studies involving sharp-lined Herbig Ae stars appear to be promising for the detection of such weak magnetic fields. These studies offer a clear spectrum interpretation with respect to the effects of blending, local velocity fields, and chemical abundances, and allow us to identify a proper sample of spectral lines appropriate for magnetic field determination. High-resolution spectropolarimetric observations of the three sharp-lined Herbig Ae stars HD101412, HD104237, and HD190073 have been obtained in recent years with the HARPS. We used these archival observations to investigate the behaviour of their longitudinal magnetic fields. To carry out the magnetic field measurements, we used the multi-line singular value decomposition method. We discovered that different line lists for HD101412 yield differences in both the shape of the Stokes V signatures and their field strengths. They could be interpreted in the context of the impact of the circumstellar matter and elemental abundance inhomogeneities on the measurements of the magnetic field. Due to the small size of the Zeeman features on the first three epochs and the lack of near-IR observations, circumstellar and photospheric contributions cannot be estimated unambiguously. In the Stokes V spectrum of HD104237, we detect that the secondary component, a T Tauri star, possesses a rather strong magnetic field <B_z>=129G, while no significant field is present in the primary component. Our measurements of HD190073 confirm the presence of a variable magnetic field and indicate that the circumstellar environment may have a significant impact on the observed polarization features.