作者: C. Catala , E. Alecian , J.-F. Donati , G. A. Wade , J. D. Landstreet
DOI: 10.1051/0004-6361:20066264
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摘要: The general context of this paper is the study magnetic fields in pre-main sequence intermediate mass Herbig Ae/Be stars. Magnetic are likely to play an important role evolution at these masses, particular controlling gains and losses stellar angular momentum. aim announce detection a structured field Ae star HD 190073, discuss various scenarii for geometry star, its environment field. We have used ESPaDOnS spectropolarimeter CFHT 2005 2006 obtain high-resolution signal-to-noise circular polarization spectra which demonstrate unambiguously presence photosphere star. Nine were obtained, each one showing clear Zeeman signature. This signature suggestive on large scales. signature, corresponds longitudinal 74+- 10 G, does not vary detectably one-year timeframe, indicating either azimuthally symmetric field, zero inclination angle between rotation axis line sight, or very long period. optical spectrum 190073 exhibits number emission lines. formation lines framework model involving turbulent heated region base wind, possibly powered by accretion. brings element our understanding magnetism masses.