The Guitar Filament’s Magnetic Field Revealed by Starlight Polarization

Jack T. Dinsmore, Roger W. Romani, Nikos Mandarakas, Dmitry Blinov and Ioannis Liodakis
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Abstract

The Guitar nebula surrounding PSR B2224+65 boasts a pulsar X-ray filament likely aligned with the local magnetic field. We present new RoboPol stellar polarization data distributed along the line of sight to the pulsar. The polarizing effect of intervening magnetized dust allows us to extract a model for the dust-weighted magnetic field. We detect a magnetic field angle consistent with the filament if the pulsar is located in the more distant zone of its parallax-estimated distance range.
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由星光偏振揭示的吉他灯丝磁场
围绕PSR B2224+65的吉他星云拥有脉冲星x射线灯丝,可能与当地磁场对齐。我们提出了新的RoboPol恒星偏振数据沿视距分布到脉冲星。磁化尘埃的极化效应使我们可以提取尘埃加权磁场的模型。如果脉冲星位于视差估计距离范围内较远的区域,我们检测到与灯丝一致的磁场角度。
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