The prevalence of weak magnetic fields in Herbig Ae stars: the case of PDS 2

• Published in: Monthly notices of the Royal Astronomical Society. Letters Vol. 449; no. 1; pp. L118 - L122
• Main Authors: Hubrig, S., Carroll, T. A., Schöller, M., Ilyin, I.
• Format: Journal Article
• Language: English
• Published: Oxford University Press 01-05-2015
• Subjects: stars: magnetic field; stars: oscillations; stars: pre-main-sequence; stars: variables: T Tauri, Herbig Ae/Be; stars: individual: PDS 2; stars: variables: general
• ISSN: 1745-3925; 1745-3933
• DOI: 10.1093/mnrasl/slv034

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 PDS 2 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 high accuracy radial velocity planet searcher (HARPS) spectropolarimetric observations of PDS 2 are used to investigate the presence of a magnetic field. A firm detection of a weak longitudinal magnetic field is achieved using the multiline singular value decomposition method for Stokes profile reconstruction (〈B
z〉 = 33 ± 5 G). To gain better knowledge of typical magnetic field strengths in late Herbig Be and Herbig Ae stars, we compiled previous magnetic field measurements, revealing that only very few stars have fields stronger than 200 G, and half of the sample possesses fields of about 100 G and less. These results challenge our current understanding of the magnetospheric accretion in intermediate-mass pre-main-sequence stars as they indicate that the magnetic fields in Herbig Ae/Be stars are by far weaker than those measured in T Tauri stars.