Non-thermal activities of highly magnetized white dwarf

中国科学院云南天文台学术报告通知

2025年第13

报告题目Non-thermal activities of highly magnetized white dwarf

报告人Jumpei Takata

报告人单位华中科技大学

报告语言English

报告时间611日(星期三)10:00-12:00

报告地点3号楼1楼会议室

报告摘要

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Rapidly spinning and highly magnetized white dwarfs have been proposed as potential sites for particle acceleration within their magnetospheres. However, definitive confirmation of such systems remains elusive.

In this presentation, I will first introduce our study on non-thermal emission from the binary white dwarf system AR Scorpii. Our findings suggest that the observed non-thermal radiation primarily originates from synchrotron emission produced by electrons at mirror points. Additionally, I will discuss our recent work exploring the possibility of non-thermal X-ray emission from isolated magnetic white dwarfs within the framework of a pulsar-like scenario.

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报告人简介:

Jumpei Takata, PhD Yamagata Unvieristy, Japan (2005). 2015 - present Professor, School of Physics, Huazhong University of Science and Techonology


云台邀请团组:星系类星体研究团组

邀请方联系人:毛基荣



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