The prevalence of weak magnetic fields in Herbig Ae stars: The case of PDS2
S. Hubrig, T.A. Carroll, M. Sch\"oller, I. Ilyin

TL;DR
This study uses high-resolution spectropolarimetry to detect weak magnetic fields in the Herbig Ae star PDS2, revealing that such stars generally have much weaker magnetic fields than T Tauri stars, challenging existing accretion models.
Contribution
First high-resolution spectropolarimetric detection of a magnetic field in PDS2, providing new insights into magnetic field strengths in Herbig Ae/Be stars.
Findings
Detected a weak magnetic field of 33±5G in PDS2.
Most Herbig Ae/Be stars have magnetic fields weaker than 200G.
Magnetic fields in Herbig Ae/Be stars are significantly weaker than in T Tauri stars.
Abstract
Models of magnetically driven accretion and outflows reproduce many observational properties of T Tauri stars, but the picture is much less clear for the Herbig Ae/Be stars, due to the poor knowledge of their magnetic field strength and topology. The Herbig Ae star PDS2 was previously included in two magnetic studies based on low-resolution spectropolarimetric observations. Only in one of these studies the presence of a weak mean longitudinal magnetic field was reported. In the present study, for the first time, high-resolution HARPS spectropolarimetric observations of PDS2 are used to investigate the presence of a magnetic field. A firm detection of a weak longitudinal magnetic field is achieved using the multi-line singular value decomposition method for Stokes profile reconstruction (<B_z>=33+-5G). To gain better knowledge of typical magnetic field strengths in late Herbig Be and…
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