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Magnetic fields of Herbig Ae/Be stars

机译:Herbig Ae / Be星的磁场

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We report on the status of our spectropolarimetric studies of Herbig Ae/Be stars carried out during the last years. The magnetic field geometries of these stars, investigated with spectropolarimetric time series, can likely be described by centred dipoles with polar magnetic field strengths of several hundred Gauss. A number of Herbig Ae/Be stars with detected magnetic fields have recently been observed with X-shooter in the visible and the near-IR, as well as with the high-resolution near-IR spectrograph CRIRES. These observations are of great importance to understand the relation between the magnetic field topology and the physics of the accretion flow and the accretion disk gas emission.
机译:我们报告了最近几年我们对Herbig Ae / Be星的光谱极化研究的现状。用分光极谱时间序列研究的这些恒星的磁场几何形状,很可能可以用具有几百高斯极性磁场强度的中心偶极子来描述。最近,在可见光和近红外以及高分辨率近红外光谱仪CRIRES中,使用X-shooter观测到了许多具有探测磁场的Herbig Ae / Be星。这些观察对于理解磁场拓扑与吸积流和吸积盘气体排放的物理特性之间的关系非常重要。

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