标题： 磁白矮星：观测、理论与未来展望 显示英文标题

标题： Magnetic White Dwarfs: Observations, Theory, and Future Prospects

摘要： 孤立磁白矮星的磁场强度范围从千高斯到吉高斯，构成了一个有趣的天体物理对象类别。磁场的起源仍然是一个热烈争论的话题。这些磁场是化石磁场（即白矮星前身恒星演化过程中被放大了的原始弱磁场）的结果，还是相反，是双星相互作用的结果，或者最终是白矮星自身演化过程中其他能产生如此强磁场的物理机制的结果，仍有待阐明。在这项工作中，我们从理论和观测两个方面回顾了白矮星磁场的现状与范式。 显示英文摘要

摘要： Isolated magnetic white dwarfs have field strengths ranging from kilogauss to gigagauss, and constitute an interesting class of objects. The origin of the magnetic field is still the subject of a hot debate. Whether these fields are fossil, hence the remnants of original weak magnetic fields amplified during the course of the evolution of the progenitor of white dwarfs, or on the contrary, are the result of binary interactions or, finally, other physical mechanisms that could produce such large magnetic fields during the evolution of the white dwarf itself, remains to be elucidated. In this work we review the current status and paradigms of magnetic fields in white dwarfs, from both the theoretical and observational points of view.