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The magnetic field of the pre-main sequence Herbig Ae star HD 190073

机译:主序序列Herbig Ae star HD 190073的磁场

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摘要

Context: .The general context of this paper is the study of magnetic fields in the pre-main sequence intermediate mass Herbig Ae/Be stars. Magnetic fields are likely to play an important role in pre-main sequence evolution at these masses, in particular in controlling the gains and losses of stellar angular momentum. Aims: .The particular aim of this paper is to announce the detection of a structured magnetic field in the Herbig Ae star HD 190073, and to discuss various scenarii for the geometry of the star, its environment and its magnetic field. Methods: .We have used the ESPaDOnS spectropolarimeter at CFHT in 2005 and 2006 to obtain high-resolution, high signal-to-noise circular polarization spectra which demonstrate unambiguously the presence of a magnetic field in the photosphere of this star. Results: .Nine circular polarization spectra were obtained, each one showing a clear Zeeman signature. This signature is suggestive of a magnetic field structured on large scales. The signature, which corresponds to a longitudinal magnetic field of 74± 10 G, does not vary detectably on a one-year timeframe, indicating either an azimuthally symmetric field, a zero inclination angle between the rotation axis and the line of sight, or a very long rotation period. The optical spectrum of HD 190073 exhibits a large number of emission lines. We discuss the formation of these emission lines in the framework of a model involving a turbulent heated region at the base of the stellar wind, possibly powered by magnetic accretion. Conclusions: .This magnetic detection contributes an important new observational discovery which will aid our understanding of stellar magnetism at intermediate masses. Based on observations obtained at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii.
机译:背景:本文的一般背景是研究主序前中间质量赫比(Herig Ae / Be)恒星中的磁场。在这些质量下,磁场可能在主前序列演化中起重要作用,特别是在控制恒星角动量的得失方面。目的:本文的特殊目的是宣布在Herbig Ae星HD 190073中检测到结构化磁场,并讨论有关星几何,其环境和磁场的各种情况。方法:我们在2005年和2006年使用CFHT的ESPaDOnS分光仪获得了高分辨率,高信噪比的圆偏振光谱,清楚地证明了该恒星光球中存在磁场。结果:获得了九个圆偏振光谱,每个光谱显示出清晰的塞曼特征。该签名暗示着大规模构造的磁场。签名对应于74±10 G的纵向磁场,在一年的时间范围内不会发生可检测的变化,表示方位角对称的磁场,旋转轴与视线之间的零倾角或旋转周期很长。 HD 190073的光谱表现出大量的发射线。我们在一个模型的框架中讨论了这些辐射线的形成,该模型涉及恒星风基部可能由磁吸积提供动力的湍流加热区。结论:该磁探测贡献了重要的新观测发现,这将有助于我们理解中等质量恒星的磁性。根据加拿大国家研究委员会在加拿大-法国-夏威夷望远镜(CFHT)上获得的观测结果,法国国家科学研究所中央科学研究院和法国大学夏威夷

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