The magnetic field and wind confinement of β Cephei: new clues for interpreting the Be phenomenon?期刊界 All Journals 搜尽天下杂志传播学术成果专业期刊搜索期刊信息化学术搜索

The magnetic field and wind confinement of β Cephei: new clues for interpreting the Be phenomenon?

Authors:	J.-F. Donati G.A. Wade J. Babel H_f. Henrichs J.A. de Jong T.J. Harries

Affiliation:	¹Laboratoire d'Astrophysique, Observatoire Midi-Pyrénées, 14 Av. E. Belin, F–31400 Toulouse, France;²Dépt. de Physique, Universitéde Montréal, CP 6128 succ Centre-Ville, Montréal QC, Canada H3C 3J7;³36 rue des Battieux, 2000 Neuchatel, Switzerland;⁴Astronomical Institute 'Anton Pannekoek', University of Amsterdam, Kruislaan 403, 1098SJ Amsterdam, the Netherlands;⁵School of Physics, University of Exeter, Stocker Road, Exeter EX4 4QL

Abstract:

Keywords:	stars: emission-line, Be stars: individual: β Cep stars: magnetic fields pulsars: general stars: rotation stars: winds, outflows