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Magnetic field detections in Herbig Ae SB2 systems

机译:Herbig AE SB2系统中的磁场检测

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Studies of the presence of magnetic fields in Herbig Ae/Be stars are extremely important because they enable us to improve our insight into how the magnetic fields of these stars are generated and how they interact with their environment, including their impact on the planet formation process and the planet-disk interaction. We report new detections of weak mean longitudinal magnetic fields in the close Herbig Ae double-lined spectroscopic binary AK Sco and in the presumed spectroscopic Herbig Ae binary HD 95881 (J?rvinen et al. 2018) based on observations obtained with HARPSpol attached to ESO's 3.6 m telescope. Such studies are important because only very few close spectroscopic binaries with orbital periods below 20 d are known among Herbig Ae stars. Our detections favour the conclusion that the previously suggested low incidence (5-10%) of magnetic Herbig Ae stars can be explained by the weakness of these fields and the limited accuracy of the published measurements. The search for magnetic fields and the determination of their geometries in close binary systems will play an important role for understanding the mechanisms that are responsible for the magnetic field generation.
机译:对Herbig AE / BE恒星中磁场的存在的研究非常重要,因为它们使我们能够改善我们对这些星星的磁场如何产生的洞察力以及它们如何与其环境进行互动,包括它们对行星形成过程的影响和行星磁盘交互。我们报告了近甲虫AE双衬里光谱二进制AK SCO中的弱平均纵向磁场的新检测,并基于用Harpspol附着在ESO的HARPSPOL获得的观察结果(J?Rvinen等,2018) 3.6米望远镜。这些研究很重要,因为在20d以下的轨道周期的眶周期仅很少的近距离光谱副杂志是Herbig AE恒星中的。我们的检测有利于先前建议的低发病率(5-10%)的磁性Herbig AE恒星可以通过这些领域的弱点和公布测量的有限精度来解释。在关闭二元系统中搜索磁场和它们的几何形状的确定将为理解负责磁场生成的机制来发挥重要作用。

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