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Large scale magnetic field of the G8 dwarf ξ Bootis A

Petit, P. ; Donati, J. F. ; Aurière, M. ; Landstreet, J. D. ; Lignières, F. ; Marsden, S. ; Mouillet, D. ; Paletou, F. ; Toqué, N. ; Wade, G. A.

In: Monthly Notices of the Royal Astronomical Society, 2005, vol. 361, no. 3, p. 837-849

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    Titel
    • Large scale magnetic field of the G8 dwarf ξ Bootis A
    Autor
    • Petit, P.. Max Planck Institut für Sonnensystemforschung, Max Planck Strasse 2, 37191 Katlenburg Lindau, Germany
    • Donati, J. F.. Laboratoire d'Astrophysique de Toulouse Tarbes, Observatoire Midi Pyrénées, 14 Avenue E. Belin, F-31400 Toulouse, France
    • Aurière, M.. Laboratoire d'Astrophysique de Toulouse Tarbes, Observatoire Midi Pyrénées, 14 Avenue E. Belin, F-31400 Toulouse, France
    • Landstreet, J. D.. Department of Physics and Astronomy, The University of Western Ontario, London, Ontario, Canada N6G 3K7
    • Lignières, F.. Laboratoire d'Astrophysique de Toulouse Tarbes, Observatoire Midi Pyrénées, 14 Avenue E. Belin, F-31400 Toulouse, France
    • Marsden, S.. Institute of Astronomy, ETH Zentrum, CH 8092 Zürich, Switzerland
    • Mouillet, D.. Laboratoire d'Astrophysique de Toulouse Tarbes, Observatoire Midi Pyrénées, 14 Avenue E. Belin, F-31400 Toulouse, France
    • Paletou, F.. Laboratoire d'Astrophysique de Toulouse Tarbes, Observatoire Midi Pyrénées, 14 Avenue E. Belin, F-31400 Toulouse, France
    • Toqué, N.. Laboratoire d'Astrophysique de Toulouse Tarbes, Observatoire Midi Pyrénées, 14 Avenue E. Belin, F-31400 Toulouse, France
    • Wade, G. A.. Royal Military College of Canada, Department of Physics, PO Box 17000, Station ‘Forces', Kingston, Ontario, Canada, K7K 4B4
    Dokumententyp
    • Postprint
    Sprache
    • Englisch
    Veröffentlicht in
    • Monthly Notices of the Royal Astronomical Society, 2005, vol. 361, no. 3, p. 837-849. Blackwell Science Ltd
    Andere elektronische Ausgabe
    OAI-PMH-ID
    • oai:doc.rero.ch:298543
    Summary
    We investigate the magnetic geometry of the active G8 dwarf ξ Bootis A (ξ Boo A), from spectropolarimetric observations obtained in 2003 with the MuSiCoS échelle spectropolarimeter at the Télescope Bernard Lyot (Observatoire du Pic du Midi, France). We repeatedly detect a photospheric magnetic field, with periodic variations consistent with rotational modulation. Circularly polarized (Stokes V) line profiles present a systematic asymmetry, showing up as an excess in amplitude and area of the blue lobe of the profiles. Direct modelling of Stokes V profiles suggests that the global magnetic field is composed of two main components, with an inclined dipole and a large scale toroidal field. We derive a dipole intensity of about 40 G, with an inclination of 35° of the dipole with respect to the rotation axis. The toroidal field strength is of the order of 120 G. A noticeable evolution of the field geometry is observed over the 40 nights of our observation window and results in an increase in field strength and dipole inclination. This study is the first step of a long term monitoring of ξ Boo A and other active solar type stars, with the aim of investigating secular fluctuations of stellar magnetic geometries induced by activity cycles