Published by
EDP Sciences
EDP Sciences Journals List
Free access
Issue A&A
Volume 442, Number 3, November II 2005
Page(s) L31 - L34
Section Letters
DOI http://dx.doi.org/10.1051/0004-6361:200500184



A&A 442, L31-L34 (2005)
DOI: 10.1051/0004-6361:200500184

Letter

Discovery of the pre-main sequence progenitors of the magnetic Ap/Bp stars?

G. A. Wade1, D. Drouin1, S. Bagnulo2, J. D. Landstreet3, E. Mason2, J. Silvester1, 4, E. Alecian5, T. Böhm6, J.-C. Bouret7, C. Catala5 and J.-F. Donati6

1  Dept. of Physics, Royal Military College of Canada, PO Box 17000, Stn Forces, Kingston, Canada, K7K 4B4
    e-mail: Gregg.Wade@rmc.ca
2  European Southern Observatory, Casilla 19001, Santiago 19, Chile
3  Dept. of Physics & Astronomy, University of Western Ontario, London, Canada, N6A 3K7
4  Department of Physics, Queen's University, Kingston, Canada
5  Obs. de Paris LESIA, 5 place Jules Janssen, 92195 Meudon Cedex, France
6  Obs. Midi-Pyrénées, 14 avenue Edouard Belin, Toulouse, France
7  Laboratoire d'Astrophysique de Marseille, Traverse du Siphon, BP 8, 13376 Marseille Cedex 12, France

(Received 25 May 2005 / Accepted 11 September 2005)

Abstract
We report the discovery, using FORS1 at the ESO-VLT and ESPaDOnS at the CFHT, of magnetic fields in the young A-type stars HD 101412, V380 Ori and HD 72106A. Two of these stars (HD 101412 and V380 Ori) are pre-main sequence Herbig Ae/Be (HAeBe) stars, while one (HD 72106A) is physically associated with a HAeBe star. Remarkably, evidence of surface abundance spots is detected in the spectra of HD 72106A. The magnetic fields of these objects display intensities of order 1 kG at the photospheric level, are ordered on global scales, and appear in approximately 10% of the stars studied. Based on these properties, the detected stars may well represent pre-main sequence progenitors of the magnetic Ap/Bp stars. The low masses inferred for these objects (2.6, 2.8 and 2.4 $M_\odot$) represent additional contradictions to the hypothesis of Hubrig et al. (2000, ApJ, 539, 352), who claim that magnetic fields appear in intermediate-mass stars only after 30% of their main sequence evolution is complete. Finally, we fail to confirm claims by Hubrig et al. (2004, A&A, 428, L1) of magnetic fields in the Herbig Ae star HD 139614.


Key words: stars: atmospheres -- stars: magnetic fields -- stars: pre-main sequence -- stars: chemically peculiar -- stars: individual: HD 72106, HD 101412, V380 Ori

SIMBAD Objects



© ESO 2005

What is OpenURL?

The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access. An OpenURL link contains article metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means.
  • If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
  • You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
  • You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.